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ADHOC software

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1. 0181 01 Lower 11 08 08 Zone 1 x1 68 000000 y1 79 000000 x2 151 000000 000000 0181 01 Lower 11 08 08 Zone 2 x1 37 000000 y1 153 000000 x2 98 000000 y2 219 000000 0181 01 Lower 11 08 08 Zone 3 x1 224 000000 y1 15 000000 x2 325 000000 y2 71 000000 0181 01 Lower 11 08 08 Zone 4 x1 346 000000 y1 77 000000 x2 440 000000 y2 141 000000 0181 01 Lower 11 08 08 Zone 5 x1 340 000000 y1 355 000000 x2 452 000000 y2 439 000000 0181 01 Lower 11 08 08 Zone 6 x1 73 000000 y1 387 000000 x2 161 000000 y2 447 000000 0181 01 Lower 11 08 09 nb pix in the 6 zones 35629 35629 0181 01 Lower 11 08 09 k tabz_ref 0 40 778103 0181 01 Lower 11 08 09 k tabz_ref 1 41 312141 0181 01 Lower 11 08 09 k tabz_ref 2 41 675987 0181 01 Lower 11 08 09 k tabz_ref 3 41 420990 0181 01 Lower 11 08 09 k tabz_ref 4 41 245373 0181 01 Lower 11 08 09 k tabz_ref 5 40 923092 0181 01 Lower 11 08 09 k tabz_ref 6 40 553814 0181 01 Lower 11 08 09 k tabz_ref 7 40 396812 0181 01 Lower 11 08 09 k tabz_ref 8 40 599205 0181 01 Lower 11 08 09 k tabz_ref 9 40 408184 0181 01 Lower 11 08 09 k tabz_ref 10 40 749821 0181 01 Lower 11 08 09 k tabz_ref 11 41 925278 0181 01 Lower 11 08 09 k tabz_ref 12 44 354233 0181 01 Lower 11 08 09 k tabz_ref
2. Suppose that you correct of these effects with the ADHOCw function B15 You will get a new ADX file which is finally a test It will be 1491 6 28713 channel 1 A and B for Y AX B 1 13856 5 83771 channel 2 and B for Y AX B 1 13556 5 70954 channel 3 and B for Y AX B 1 13716 5 77753 channel 4 and B for Y AX B 1 13925 5 86712 chan 5 A and B for Y AX B D gt PS 5 0 1345 5 6654 channel 6 A and B for Y AX B 13815 5 8198 channel 7 A and B for Y AX B 13691 5 76748 channel 8 A and B for Y AX B 1382 5 82134 channel 9 A and B for Y AX B 13664 5 75597 channel 10 A and B for Y AX B 13615 5 73435 channel 11 A and B for Y AX B 13693 5 7684 channel 12 A and B for Y AX B 1 13916 5 86309 channel 13 A and B for Y AX B 1 14296 6 02491 channel 14 A and B for Y AX B 1 13863 5 84072 channel 15 A and B for Y AX B 1 13714 5 77738 channel 16 A and B for Y AX B 1 13726 5 78197 channel 17 A and B for Y AX B 1 14985 6 31892 channel 18 A and B for Y AX B 1 14439 6 08583 channel 19 A and B for Y AX B 1 13708 5 77425 channel 20 A and B for Y AX B 13581 5 72021 channel 21 A and B for Y AX B 13936 5 87165 channel 22 A and B for Y AX B 13178 5 54861 channel 23 A and B for Y AX B 14082 5 93448 channel 24
3. f4 2D input file 04 name with whole path 00 5 2D input file 05 name with whole path 000 f6 2D input file 06 name with whole path 000 f7 2D input file 07 name with whole path f8 2D input file 08 name with whole path f9 2D input file 09 name with whole path file C ADHOCw HELP adwt1_h4 htm 3 of 4 15 02 02 09 34 59 ADwT1 tuning 10 2D input file 10 name with whole path 0 f1 2D input file 11 name with whole path 0 12 2D input file 12 name with whole path 000 13 2D input file 13 name with whole path 00 14 2D input file 14 name with whole path 0 15 2D input file 15 name with whole path 000 ml ml nl ll Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h4 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_h4 htm 4 of 4 15 02 02 09 34 59 ADwT 1 Peculiar corr
4. keyword content options MINMAX fin 2D or 3D input file name with whole path Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0230 02 Lower 2 32 04 Input file is 3D 0230 02 Lower 2 32 11 Nb of not masked pixels 7077888 0230 02 Lower 11 32 11 Nb of NULL lt 3 0E38 pixels 0 0230 02 Lower 11 32 11 Mini 32763 000000 i 1 j 401 k 8 0230 02 Lower 2 32 11 Maxi 32765 000000 i 1 j 254 k 15 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser file C ADHOCw HELP adwt1_b4 htm 2 of 3 15 02 02 09 34 38 ADwT1 maximum and minimum incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b4 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b4 htm 3 of 3 15 02 02 09 34 38 ADwT1 arithmetic operations ADwT1 Return to main ADHOCw help Return to main ADwT1 help B05 Arithmetic operations on 2D or 3D files Input 20 or 3D file F1 Output 20 or 30 file F2 Arithmetic ope
5. 1 0 e 0 999896 0 channel 4 A and B for Y AX B 0 99989 0 channel 5 A and B for Y AX B 0 999917 0 channel 6 A and B for Y AX B 0 999795 0 channel 7 A and B for Y AX B 0 999778 0 channel 8 A and B for Y AX B 0 999921 0 channel 9 A and B for Y AX B file C ADHOCw HELP adwt1c1 1 htm 6 of 8 15 02 02 09 34 53 ADwT1 rough photometry 999944 0 channel 10 A and B for Y AX B 999861 0 channel 11 A and B for Y AX B 999892 0 channel 12 A and B for Y AX B 99988 0 chann 999852 0 chan 99984 0 chann 13 A and B for Y AX B el 14 A and B for Y AX B 15 A and B for Y AX B 999816 0 channel 16 A and B for Y AX B 999906 0 channel 17 A and B for Y AX B 999968 0 channel 18 A and B for Y AX B 999949 0 channel 19 A and B for Y AX B 999832 0 channel 20 A and B for Y AX B 999892 0 channel 21 A and B for Y AX B 999864 0 channel 22 A and B for Y AX B 1 23 A and B for Y AX B el 24 A and B for Y AX B 25 A and B for Y AX B 99981 0 chann 999864 0 chan 99982 0 chann Sf pS Sa So S amp S D 9 SP Sp Bb 5 a Ss D D Bs 8 L i 1 OOO COO Oo Oo Oo Oo OO Oo Oo OC Oo OC Oo Oo Oo Oo OO Oo Oo Oo Oo Oo Oo Oo Oo Oo Oo Oo Oo Oo Oo OO oO O 999898 0 channel 26 A and B for Y AX B 999827 0 channel 27 A and B for Y AX B 999778 0 channel 28 A and B for Y AX B 9
6. e oe I Oo OF NN FE A I 1 amp NN OH A A A En pa co o N N A IDD IIIII1 D D A A Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for file C ADHOCw HELP adwt1_c9 htm 4 of 5 15 02 02 09 34 52 ADwT1 Finesse extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c9 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_c9 htm 5 of 5 15 02 02 09 34 52 ADwT1 rough photometry ADwT1 Return to main ADHOCw help Return to main ADwT1 help C11 Get photometric parameters from non dephased channels CCD su ADHOCw rough photometry ADHOCw Gel photomeine parameters fan AGA Pephased ChERRE S fusetul for CCS Input original not dephased 30 file Choose file ID DatalKlineb2_cos ad3 Input 602 SSC zones input file Choose file D DatalKizones 2 adz Output Abie ASCH photometric parameters tile Choose file D DataUKltruc ade M Use an input 20 reference photometric file 20 photometric reference file Choose file Output control BMP Choose file D Da
7. ff yee PR leviovereti A masie Renbow El MEMEUCEC TalENIES j MISES 1 file C ADHOCw HELP adw2dd2t htm 15 02 02 09 33 52 ADw2D cross sections ADw2D Return to main ADHOCw help Return to main ADw2D help Cross sections Cross section mode The default mouse action mode is the cross section mode But you must check that the cross section mode is running in the Action of the left button of the mouse box If not simply press the corresponding radio button The thickness box will appear Action of the left button of the mouse Cross sections Integration of profile Image modification te Tiesboveray gt Kinematcs oraalevies te Histogram Mini 0 000000 Maxi 4109605957 C Cross section parameters Thickness 0 a pixels Cross section procedure To do a cross section simply click the left mouse button at the location of one extremity of the desired cross section Then click again on the other extremity The cross section drawing appears on the top right location of the window When you move the mouse inside the drawing you can get the X and content values of the cross section A simultaneous second cursor on the image indicates the exact correspondence between the cross section position and the image position At the same time the zoom fits with the exact location of the cross section You can also change the drawing scale by editing directly the mi
8. current cycle 0000 0099 SSS dons THT ct ENDES pre ss scanning wavelength 6562 780 Abort and Quit x RIT ER RER Standby object Queensgate constant 2 3350 Shutter Cumulated Reguest deferred stop WE open Instantaneous exposure time 00 00 00 System priorities automatic from photon rate photons s 842 total nb photons 000000000000 High a maxphis UNIT r frames s 25 written on disk 0000000 0 Mb Critic r z count efficiency100 total counting efficiency 0 TV parameters EB allow modification Discri Ro Black lvl e of the TV parameters def 20 def 51 file C ADHOCw HELP adwi_gen htm 15 02 02 09 34 04 ADwIPCS tuning ADwIPCS Return to main ADHOCw help Return to main ADWIPCS help Tuning the system before acquisition The level determination is very important it changes even during one night and the user must check in permanence that the efficiency of the system is maximum This can be done by looking regularly to the second TV VGA monitor which displays the work of the MATROX board But the user must check carefully every thing before the observation AD ADHOCw Test Matrox Genesys Board and Imaging Library HIL ADHOCw Test Matrox Genesys Board and Imaging Library MIL Some of these test and demonstrations functions of the Matrox Genesys board require an additional screen display which must be connected on the VGA plug of the Matrox Genesys board The programs which require thi
9. lo db I a au u 409 i 10 j 1 i 11 j 1 102 i 12 j 1 625 i 13 j 1 131 i 14 j 1 i 15 j 1 i 16 j 1 i 17 j 1 0 0 0 0 0 2 5 8 10 i 9 j 1 8 5 2 0 0 0 0 0 The number of values must be 17 Number of spaces is not important and and all what is on right can be suppressed For compatibility for similar files smoothing in X and Y j 1 is mentioned Macro definition Example SMOOTHZ fin D ADHOCws_plus BLAISOUS Call da3 fout D ADHOCws_plus BLAISOUS bidon ad3 square 3 keyword content options note fin 8D input file name with whole path p fout 3D output file name with whole path square nbofbinnedadjacentchannels 5ee Note 1 below i ee ES lorentz half maximum width in channels see Note 1 below 4 gt detail other 5 gt edge enhance user user file containing the filter values see Note 1 below l gt smooth 1 gt smooth 2 gt blur 3 gt sharpen see Note 1 below Note 1 square gauss lorentz other and user options exclude themselves file C ADHOCw HELP adwt1_b8 htm 3 of 4 15 02 02 09 34 40 ADwT1 spectral smoothing Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simp
10. Direct 2D files versus ADC contexts General functions Main 2D display screen Composition with several 2D images blink Cross sections Image modification Graph superposition and modification of 3D profiles Superposition of text and drawings Kinematical functions This program requests a minimum screen of 1024x768 with 256 colors and 96 pixels per inch If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode Comment or information boulesteix observatoire cnrs file C ADHOCw HELP adw2d htm 2 of 3 15 02 02 09 33 47 ADw2D 2D display module mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhoc help adhocw htm file This file is adw2d htm Return to main ADHOCw menu file C ADHOCw HELP adw2d htm 3 of 3 15 02 02 09 33 47 ADw2D direct files and ADC contexts ADw2D Return to main ADHOCw help Return to main ADw2D help Direct 2D files versus ADC contexts The following window is the first window to be displayed when the ADw2D exe program is called ADHOCw 2D display J Bouleste
11. file C ADHOCw HELP adwt1_c htm 3 of 3 15 02 02 09 34 51 ADwT1 monochromatic continuum RV maps ADwT1 Return to main ADHOCw help Return to main ADwT1 help C03 Computation of the monochromatic continuum radial velocities and widths 2D maps ADw mono R OF X ADHOCw maono cont RY widths Algorithms Type of line emission v Input 3D file Profile analysis Output suffis name forc 1 to 16 characters Slope change recommended 2 Nb of successive chnls Output 2D file monochromatic image Choose file DADHOCwS_plus BLAISOUS Mono_ORG AD2 Output 2D file continuum image Choose file Fixed levels D ADHOCws_plus BLAISOUS Cont_ORG AD2 Rs H VS eee Output 2D file Radial Velocities Choose file D ADHOCws_plus BLAISOUS VR_ORG AD2 Continuum computation Output 2D file line widths GRR Mean of the 3 lowest channels D ADHOCws_plus BLAISOUS Width_ORG AD2 From intensity histogram fi 0 Continuum channels f Execute Help x Abort Store macro Value of the lowest channel As for the old ADHOC the program proposes to give the same file name end Output suffix name to the 4 x 2D files which are created You can easily edit this output suffix name and the effect will be immediately seen on the file names themselves The type of line to measure can be emission or absorption There are two profile analysis methods slope change the parameter nb of suc
12. radial velocities 642 633 623 614 604 595 585 975 566 9 9 6 547 p 528 518 509 99 89 80 70 61 Sle 42 B26 23 134 04 394 71 92 13 34 55 75 96 17 38 59 80 01 22 43 64 85 05 26 47 68 89 10 31 52 73 94 15 2 85 28 73 18 64 09 52 97 42 87 33 76 yad 66 PR 54 99 45 90 35 78 23 69 14 59 02 47 6554 6554 6554 6554 6955 6555 6555 6555 6556 6556 6556 6556 6556 6557 6557 6557 6557 6527 6558 6558 6558 6558 6558 6559 65 59 6559 6559 384 315 2365 356 346 331 3241 816 308 298 28 9 LAD 2 10 260 251 241 232 222 212 208 193 184 174 165 ESOK 146 136 6562 78 Angstroems for 0 00 km s 5 65 Angstroems 257 92 km s 0 21 Angstroems 9 55 km s 35 56 77 98 19 40 61 82 03 24 45 65 86 07 28 49 70 91 12 33 54 75 95 16 37 58 79 1 92 38 81 26 71 16 61 04 50 95 40 83 28 74 19 64 07 52 97 43 88 31 76 21 67 09 59 6571 64 Angstroems 6560 6560 6560 6560 6560 6561 6561 6561 6561 6561 6562 6562 6562 6562 6562 6563 6563 6563 6563 6563 6564 6564 6564 6564 6565 6565 6565 127 117 107 296 88 7 9 69
13. 0 00 nOAAAOAAROARRAAADOAARAKAMRAARDAAARAAADAAASSAAAAE The user can edit the additional points which will not be drawn but will be taken in account during the computation of the curve Note that the weight must be coherent with the weight of the points which is always 1 in points mode or the weight of the crowns which is proportional to the number of valid velocities integrated in each crown Save coefficients values as TXT allows to save the coefficients of the curve in a TXT file Create 2D image from the curve creates a 2D file with the theoretical velocity field corresponding to the computed curve Create 2D residuals from the curve creates a 2D file with the deviation V_real V_theoretical obtained from the 2D file 01 V real and the curve V theoretical file C ADHOCw HELP adwa2d_k1 htm 8 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph Superposition of r V plots The r V plots are isophotes which represent a cross section along the major axis Only pixels which lie in a narrow band along the major axis are taken in account Then their p see Rotation velocities radial velocities projected rotation upper for definition of p is computed and plotted as r The value of the isophote at a given velocity is the integration of the corresponding channel values at these points A 3D file is needed the 3D file 11 is always taken Draw from 3D file 11 if this box is checked the
14. 0272 O01 Lower 10 31 05 Chnl 4 New A Old B A 1 293210 10 474100 0272 O01 Lower 10 31 05 Chnl 5 New A Old B A 1 123900 9 615320 0272 01 Lower 10 31 05 Chnl 6 New A Old B A 1 212280 2 670230 0272 O01 Lower 10 31 05 Chnl 7 New A Old B A 0 987761 9 150510 0272 O01 Lower 10 31 05 Chnl 8 New A Old B A 1 168820 7 52532 Q 0272 0l Lower 10 31 05 Chnl 9 New A Old B A 1 201140 2 723190 0272 O01 Lower 10 31 05 Chnl 10 New A Old B A 1 23074 7 107360 0272 0O1 Lower 10 31 05 Chnl 11 New A Old B A 1 10415 8 040110 0272 O01 Lower 10 31 05 Chnl 12 New A Old B A 1 02561 B 5 417010 0272 O01 Lower 10 31 05 Chnl 13 New A Old B A 1 12552 15 855700 0272 01 Lower 10 31 05 Chnl 14 New A Old B A 1 00803 B 0 120650 0272 01 Lower 10 31 05 Chnl 15 New A Old B A 1 12978 1 286880 0272 01 Lower 10 31 05 Chnl 16 New A Old B A 1 13325 2 659480 0272 01 Lower 10 31 05 Chnl 17 New A Old B A 1 17313 10 086500 0272 01 Lower 10 31 05 Chnl 18 New A Old B A 1 21033 0 606203 0272 O01 Lower 10 31 05 Chnl 19 New A Old B A 1 04791 7 439380 0272 O01 Lower 10 31 05 Chnl 20 New A Old B A 1 15636 5 364240 0272 0l1 Lower 10 31 05 Chnl 21 New A Old B A 1 27735 8 603450 0272 O01 Lower 10 31 05 Chnl 22 New A Old B A 1 23585 6 188370 0272 O01 Lower 10 31 05 Chnl 23 New A Old B A 1 09640 6 140290 0272 01 Lower
15. 1 11 dau a ides sh Mass a I by Awe beer xp Ex 38 CETTE CRUE Jax by Lam L art Eee 4 LIN 2 EEN DELL Lis Le Tit red cox E E 4x0 4x0 Westonte walt fia 4p m E ETET 4 Sess ove se Hand C C mx Sw 2 J un sun w erfa l As mar alle oy Ucan j The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens to visualize the figure with full resolution for help manual on paper see next page Preliminary note the kinematical functions work exclusively on the 2D file 01 and if necessary on the 3D file 11 This assignation is implicit The data of other files are never taken in account except normal display and 2D file 02 in case of masking In case of masking if the 2D file 01 is masked by the 2D file 02 the masked values velocities are not taken in account Parameter file the parameter file is of ADK type special for kinematics ASCII Load parameter file loads a previous ADK file and displays the results Sets the automatic saving function on Save parameters to file saves kinematical parameters into a ADK file file C ADHOCw HELP adw2d_k htm 3 of 6 15 02 02 09 34 24 ADw2D kinematical functions Automatic saving if this checkbox is checked the parameters file will be saved at any modification of the parameters Center of rotation it is usually the center of rotation Floati
16. Image Extension a N dimensional array of pixels like in a primary array ASCII Table Extension rows and columns of data in ASCII character format Binary Table Extension rows and columns of data in binary representation In each case the HDU consists of an ASCII Header Unit followed by an optional Data Unit For historical reasons each Header or Data unit must be an exact multiple of 2880 8 bit bytes long Any unused space is padded with fill characters ASCII blanks or NULs depending on the type of unit Each Header Unit consists of any number of 80 character keyword records or card images reminiscent of the 80 column punched cards which were prevalent when the FITS standard was developed which have the general form KEYNAME value comment string The keyword names may be up to 8 characters long and can only contain uppercase letters the digits 0 9 the hyphen and the underscore character The keyword name is usually followed by an equals sign and a space character in columns 9 10 of the record followed by the value of the keyword which may be either an integer a floating point number a character string enclosed in single quotes or a boolian value the letter T or F The last keyword in the header is always the END keyword which has no value or comment fields There are many rules governing the exact format of a keyword record see the NOST FITS Standard so it is better to rely on standard interface software like F
17. Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_c htm Return to main ADHOCw menu Return to main ADWFT menu file C ADHOCw HELP adwft_c htm 2 of 2 15 02 02 09 34 09 ADwFT Macros and batch ADwFT Return to main ADHOCw help Return to main ADWFT help Macros and batch As for the ADwT1 program the user has access to macros that can be executed sequentially later fi ADWFT MEE TP TR de E TT ee a Ofte ADHOCw File Translator EL El E a Presentation 3D gt 3D 2D gt 2D 3D gt 2D slices 2D slices gt 3D File parameters Dump and modify Macros Function This function allows to run automatically an ASCII file containing successive commands for translations Each line corresponds to the translation of one file Instructions INSTRUCTIONS FOR THE ADHOCw FILE TRANSLATOR MACROCOMMANDS A amp A macro command file is an ASCII file containing macro commands These macro commands are C type commands they may continue on several lines they are always terminated by parameters are separated by space s The default extens
18. Version 2000M 13 nov 2000 adwt1 new function B17 2D or 3D mosaic Version 2000L 06 nov 2000 adw3d now managing floats 4 bytes for data reduction and short integers 2 bytes for data acquisition adwt1 new function HO9 Perot Fabry characteristics and Queensgate constants adwt1 new function H10 common nebular and calibrations wavelengths Version 2000K 18 oct 2000 adwt1 new functionH06 precessions and object visibility adwt1 new function H07 sideral time clock adwt1 new function HO8 interference filters adw2d possibility to display external rotation curves Version 20001 19 jul 2000 adw2d adwsbD assigning file extensions to ADHOCw programs in order to open files directly from the Explorer Version 2000H 19 jun 2000 adw2d user made crown sectors for kinematical analysis free r PA Vs incli adw2d optimization of the basic kinematical parameters MA Vs and incli Version 2000G 01 jun 2000 adwt1 new function C11 to analyze CCD photometry creating an ADX file with only one variable transparency for example Version 2000D 12 may 2000 file C ADHOCw HELP adw_new htm 2 of 3 15 02 02 09 35 04 ADHOCw new in the last versions adwt1 global batches ADB files chaining local batches in different directories Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple
19. 0173 01 Lower 17 58 19 k tabz_ref 29 912 410828 0173 01 Lower 17 58 19 k tabz_ref 30 912 415527 0173 01 Lower 17 58 19 k tabz_ref 31 912 427490 0173 01 Lower 17 58 19 k tabz ref 32 912 459229 0173 01 Lower 17 58 19 k tabz_ref 33 912 577087 0173 01 Lower 17 58 19 k tabz_ref 34 912 599121 0173 01 Lower 17 58 19 k tabz ref 35 912 571655 0173 01 Lower 17 58 19 k tabz_ref 36 912 614807 0173 01 Lower 17 58 19 k tabz_ref 37 912 673584 0173 01 Lower 17 58 19 k tabz ref 38 912 645996 0173 01 Lower 17 58 19 k tabz_ref 39 912 669434 0173 O01 Lower 17 58 19 k tabz_ref 40 912 611084 0173 01 Lower 17 58 19 k tabz_ref 41 912 702515 0173 01 Lower 17 58 19 k tabz_ref 42 912 645508 0173 01 Lower 17 58 19 k tabz_ref 43 912 669250 0173 01 Lower 17 58 19 k tabz_ref 44 912 756165 0173 O01 Lower 17 58 19 k tabz_ref 45 912 714172 0173 01 Lower 17 58 19 k tabz_ref 46 912 754822 0173 01 Lower 17 58 19 k tabz ref 47 912 763916 0173 01 Lower 17 58 19 Correct end 0173 O01 Lower 17 58 19 Ending function Expected results Suppose that you look to a normal CCD CFHT observation The analysis with this function will give an ADX file which is for instance The following correction values are from the tabz_ref values above val val_min 99999 0 channel 1 A and B for Y AX B 0 channel 2 A and B for Y AX B 99995 0 channel 3 A and B for Y AX B
20. 0182 16 Batch Lower 18 16 28 G01 2 441 channels 0182 16 Batch Lower 18 16 28 G01 2 117 channels 0182 16 Batch Lower 18 16 28 G01 1 794 channels 0182 16 Batch Lower 18 16 28 G01 1 469 channels 0182 16 Batch Lower 18 16 28 G01 1 146 channels 0182 16 Batch Lower 18 16 28 G01 0 823 channels 0182 16 Batch Lower 18 16 28 G01 0 499 channels 0182 16 Batch Lower 18 16 28 G01 0 175 channels 0182 16 Batch Lower 18 16 28 G01 0 148 channels 0182 16 Batch Lower 18 16 28 G01 0 472 channels 0182 16 Batch Lower 18 16 28 G01 0 797 channels 0182 16 Batch Lower 18 16 28 G01 1 120 channels PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info file C ADHOCw HELP adwtt_g1 htm 8 of 14 15 02 02 09 34 36 order 584 order 585 order 586 order 587 order 588 order 589 order 590 order 591 order 592 order 593 order 594 order 595 order 596 order 597 order 598 order 599 order 600 order 601 order 602 order 603 order 604 deviation deviation deviation deviation deviatio
21. 4712 066 4715 346 4788 927 4827 344 4884 917 4957 033 5330 777 5341 094 5343 284 5400 562 5764 419 5852 488 5881 895 5975 534 6029 997 6074 338 6143 062 6163 594 6217 281 6266 495 6334 428 6382 991 6402 246 6598 953 6929 467 7032 413 7173 938 7245 166 8300 325 8495 359 8634 647 8654 384 8679 490 8681 922 8780 622 8783 754 8853 877 8865 756 9148 68 9201 76 9300 85 9326 52 9425 38 9486 680 A 9534 167 9665 424 10562 43 10844 54 11143 09 11177 59 18276 59 18282 58 18385 17 Do no De Do Do Do Do Do Do Do Je Do po D Do Do Do Do Do Do Do Do Je Do po D Do Do Do Do Do Di Do Do Je Do po D De De peo Do Do Poo file C ADHOCw HELP adwt1h10 htm 2 of 3 15 02 02 09 35 04 ADwT1 Common wavelengths H lium He I 3888 648 A 4471 479 A 5015 678 A 5875 691 A 5875 966 A 6678 151 A 7065 190 A 10829 088 A 10830 248 A 10830 337 A 17002 38 A 18685 96 A 18696 94 Sodium 4541 633 5889 950 8649 922 10749 29 11403 78 4324 615 4390 029 4393 340 Na I 4423 246 4494 177 4497 658 4545 186 5688 205 A 5895 924 DEL 284 10834 87 8194 824 10746 44 11381 45 Do Do Do Do 14767 48 22056 44 Log book results None Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the
22. 90 40 30 20 10 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 21 24 27 30 33 36 ES LS 15 LE TS I5 LS LSe 15 15 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 61 64 67 70 Taa 76 29 55 9 9 Jon 55 55 Jor 55 55 55 00 00 00 00 00 00 00 00 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 30 30 30 30 30 30 30 30 30 00 30 00 30 00 30 00 30 00 30 00 30 00 30 00 PRO I Oo OB RH 00 0 00 15 00 55 00 2320 00 30 00 12 0 00 10 00 18 00 58 00 2320 00 30 00 13 2320 2320 2320 2320 2320 2320 2320 2320 00 1 00 TL 00 1 00 1 00 1 00 19 00 20 00 21 1 oO U1 A 100 00 15 00 55 00 2320 00 30 00 22 100 00 110 00 15 00 55 00 2320 00 30 00 23 110 00 120 00 15 00 55 00 2320 00 30 00 24 file C ADHOCw HELP adw2d_k2 htm 5 of 12 15 02 02 09 34 27 the successive sectors are linked Overlapping crowns are not correct in this case the pixel Lis selected only in the first crown Note 3 If you press Create a regular array with the fixed parameters you get the same drawings as in classical mode without defined crowns but you can minimize PA r Ys r and incli r Last column number of the crown ADw2D kinematical functions user m
23. C ADHOCw HELP adw_what htm 4 of 15 15 02 02 09 33 45 ADw what is ADHOCw Coordinates The coordinates are numbered from 1 never from 0 in ADHOCw For instance in a 256 x 256 x 24 cube the valid user coordinates are 1 to 256 in X and Y and 1 to 24 in Z Input and output data file types Program Accepted input file types Created output file types ADw2D new ADHOCw AD2 AD3 new ADHOCw AD2 AD3 old ADHOC DA2 DA3 FITS any type ADw3D new ADHOCw AD2 AD3 new ADHOCw AD2 AD3 FITS any type ADwT1 new ADHOCw AD2 AD3 new ADHOC AD2 AD3 old ADHOC DA2 DA3 ADWFT new ADHOCw AD2 AD3 new ADHOCw AD2 AD3 old ADHOC DA2 DA3 old ADHOC DA2 DA3 FITS any type FITS any type IDL and binary any type IDL and binary any type ElCcompressed Chile EIC compressed Chili ADwIPCS new ADHOCw AD2 AD3 new ADHOCw AD2 AD3 old ADHOC DA2 DA3 FITS any type IPCS coordinates ADA CIG Read the new ADHOCw format characteristics the old ADHOC format characteristics the FITS format characteristics the IDL binary format characteristics ADHOCw files formats and suffixes All ADHOC files accept long names up to 256 characters including the path The extension must be less than 30 characters All ADHOC files can be shared and read or written from other computers through the network Suffix Type of file Type of data Description AD1 1D data profile ASCII cl
24. Macro definition Example Macro PECULIAR CORR fin D Data Godbout 512_512 calib ad3 fout D Data Godbout 512_512 un ad3 oper 1 keyword content options PECULIAR_CORR 3D input file name with whole ins path 3D output file name with whole f2 path oper operation mode 0 Megantic scanning shift 1 Megantic scanning interpolation Log book results Excepted the text of the macro and the ending execution message no information is recorded file C ADHOCw HELP adwt1_h5 htm 2 of 3 15 02 02 09 35 00 ADwT1 Peculiar corrections Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h5 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h5 htm 3 of 3 15 02 02 09 35 00 ADwT1 Precessions ADwT1 Return to main ADHOCw help Return to main ADwT1 help H06 Precessions and object visibility 9 ADw Precessions and object visibility Iof x ADHOCw _ Object name th dm 5 deg epoch i gy O DEOL 3 de 740 a o 3
25. Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC file C ADHOCw HELP adwa2d_d htm 2 of 3 15 02 02 09 33 52 ADw2D cross sections But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2dd_d htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_d htm 3 of 3 15 02 02 09 33 52 ADw2D Cross section full size EF Export display to BMP B Setup printer BP Print S Save ADC context Help XM Quit the prograny Parameters Image file C ADHOCw HELP adwadi2t htm 15 02 02 09 33 53 sf Mouse arga 1 zoom 19x19 pix Cursor 1x1 pix Mouse area 2 E Whole image vr Display parameters Flip vertivally Print values x Val EES Flip horizontally Graph area i Frs E Rainbow eves area Visualization mode Square pixels File 1 File 2 Scale max 1120 Threshold 0 01 01 1 10 10 100 100 1000 1000 01 01 1 1 10 10 100 100 1000 1000 Scale min 0 Scale overlap Actualize full display Lines Lines Y Had IN one Y None mi 2 Action of the left button of th
26. Note 2 It is recommended to have crowns increasing radii in order to get a correct drawing of the sectors the drawing of the successive sectors are linked Overlapping crowns are not correct in this case the pixel is selected only in the first crown Note 3 If you press Create a regular array with the fixed parameters you get the same drawings as in classical mode without defined crowns but you can minimize PAfr s r and inclifr file C ADHOCw HELP adw2d_k2 htm 3 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns There is the possibility to define up to 256 crown sectors r min p is the minimal distance in pixels to the center of the crown sector in sky polar coordinate p r max p is the maximal distance in pixels to the center of the crown sector in sky polar coordinate p PA min p is the minimal position angle in degrees in sky polar coordinate 6 PA max p is the maximal position angle in degrees in sky polar coordinate 6 Vs p is the systemic velocity in km s incli p is the inclination in degrees with respect to the sky plane The user can load a previous ADV file containing the parameters of the crown sectors He can also save the crown sectors parameters into a ADV file The user can also redefine a set of crown sectors from fixed parameters and then edit them At any moment the user can edit the array D ADw2D ADV edition lolx ADw2D A
27. Return to main ADHOCw help Return to main ADwT1 help H08 Interference filters file C ADHOCw HELP adwt1_h8 htm 1 of 6 15 02 02 09 35 02 ADwT1 Interference filters ADw Interference filters Tal ADHOCW Aiter selection Etter Sat soure Read fiter list file c adw_lf tmp Previous call list 144 filters read Help ADHOCw generic filter list y Enora ee ori Click on the active sum to aii se a ne Apan BEER 410 000 1510 oo 23 00 KG LE RE i i 6569 80 1000 3300 920 000 2300 167 400 562 2 F 3 JN 6582 90 980 55 30 940 000 2300 14 67 400 562 2 i 4 jn 658970 910 5900 940 0 00 2300 4167 400 562 2 e 5 y 655870 910 6400 910 0 00 2300 167 4 00 5 62 FA lit HE N 6581 20 10 30 6400 9 30 0 00 2300 1 67 400 5 62 zi i N 656550 1110 5850 940 000 2300 167 400 562 2 it 8 N 656560 460 5300 1020 O00 2300 167 400 562 2 is 9 IN 6576 20 11 20 5680 930 000 2250 167 400 562 2 i N 6568 10 530 4550 930 O00 2350 167 400 562 2 i N 6570 20 450 4900 890 OOO 2300 167 400 562 2 i N 6575 80 490 5800 9320 0 00 2300 4 67 400 562 2 Hn N 656710 980 5250 1140 000 2300 167 400 562 2 iE Y 6594 60 620 5900 1100 000 2300 167 400 562 2 i 16 Jy 6597 70 950 7000 1080 000 2300 167 400 562 2 tie Y 6574 00 970 71 00 1060 000 2300 167 400 562 2 i Y 661264 400 5550 10 60 000 2300 4 67 400 562 2 ii Y 6563 00 300 6000 970 OOO 2300 167 400 562 2 verifier Y 6583 00 1200 6200 1040 000 2000 167 400 562 2 verifie
28. gt smooth user user file containing the filter values see Note 1 below 2 gt blur see Note 1 below 3 gt sharpen Note 1 square gauss lorentz other and user options exclude themselves Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite file C ADHOCw HELP adwt1_b9 htm 5 of 6 15 02 02 09 34 42 ADwTI spatial smoothing HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b9 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwtt_b9 htm 6 of 6 15 02 02 09 34 42 ADWT1I figure BO9 full size ADw smoothing file C ADHOCw HELP adwt1 b9t htm 15 02 02 09 34 42 ADwT1 rotation scaling XYZ translations ADwT1 Return to main ADHOCw help Return to main ADwT1 help B11 Rotation scaling XYZ translation and inversion for 2D or 3D files rb ADw translation ro
29. nl enregistrements nl dimension Y ydim de npl valeurs npl dimension X xdim 1 valeur 2 octets integer 2 b structure des fichiers 3 D de type xxxxxxxx DA3 n enregistrements n nl npl nb de pixels xdim ydim de m valeurs m dimension Z nb de canaux 1 valeur 2 octets integer 2 c fichier parametre 2 D de type Xxxxxxxx Il est cree par VISU2 s il n existe pas Ce fichier ASCII est imprimable et peut etre edite Il contient 2 4 lignes ligne 1 dimension X dimension Y xdim ydim format libre _ ligne 2 commentaire 78 caractSres maxi format a78 ligne 3 sauvegarde des niveaux de visualisation del image par VISU2 ligne eventuelle automatiquement creee si absente Format libre contient 12 valeurs seuil pas palette mode visualisation mode logarithmique zoom par rapport a 256 Xo coin HG fenetre Yo coin HG fenetre seuil isophotes superposees pas isophotes superposees nombre d isophotes superposees limite de qualite masquage ligne 4 sauvegarde des inhibitions de niveaux de visualisation de VISU2 ligne eventuelle automatiquement creee si absente Format libre contient 15 valeurs d fichier parametre 3 D de type xxxxxxxx 3 Il peut ventuellement etre cree par la fonction ADHOC No 74 s il n existe pas Ce fichier ASCII est imprimable et peut etre edite Il contient 5 lignes ligne 1 idim icarre ix1 ix2 iy1 iy2 nc idim dimension TOUJOURS 3 icarre
30. the scale of the graph can be less than 100 In this case the fonts and symbols are not undersampled as classical programs as paint do when they resize an original image Frame Symbols Digits jv aoled Fi saints open square filled square Draw symbols in crowns mode if this box is checked the symbols bars are drawn Draw error bars in crowns mode if this box is checked the error bars are drawn mean deviation Equidistant r crowns in crowns mode if this box is checked the symbols on every side blue and red appear at the same r location This esthetic drawing is discutable because the r drawn is not the exact r mean r of all the points but the geometric center of the crown file C ADHOCw HELP adw2d_k1 htm 4 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph Graph in black for publication all the symbols and curves are no more drawn in color but in black Bold RV points in points mode the individual velocity points are bold is this box is checked Symbol size width of the drawn symbols in screen points Line width of the drawn line of the symbols in screen points Error bar width width of the drawn line for error bars open square filled square cross X cross open circle filled circle blue symbol can be no symbo open square filled square cross X cross open circle filled circle red symbol can be no s
31. 0003 01 Lower 18 31 31 Writing result 0003 01 Lower 18 31 42 Global statistics on photons 0003 01 Lower 18 31 42 Nb photons of remanence with 0 pixel hift 40145 16 5 0003 01 Lower 18 31 42 Nb photons read 244011 remnants 0145 final 195406 80 1 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_e1 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_e1 htm 5 of 5 15 02 02 09 34 06 ADwTI1 batchs ADwT1 Return to main ADwT1 help Batches There are two ways to execute ADHOCw ADWwT1 functions the direct execution by pressing the Execute button or the deferred batch execution by pressing the Store macro button The file in which macros can be stored is an ASCII file of ADM suffix AHOHCw macro This ADM file can be edited easily by the user in order to generate new sequences The store macro button leads the user to this window ADw macro record Ioj x ADHOCw Recording a macro File containing the macros ADM Choose file Present content of
32. 15 02 02 09 34 23 Overlays 0 xj igs ea ur ak Ta Tae Ta Disk Lime I FillRect Blue Add new component Suppress one component B3 Text Fuchsia This is z227 4 Text Yelow inclined 349 Yellow 7 BE riai mecs 250 400 9 lt 2 179 282 16 430 490 24 0 16 45 345 426 sc TE 4 Text and overlays Export to Clipboard Fa 7 Swap to coord Export display to BMP Print S _ictualize full display Fa Save ADC contest Help Return to main Adding one component amp Dw2D add or edit an overlay component oj x Component 1 Type Disk Color Lime Width v FCircle fine width ParameterA 200 FCircle X1 position Parameter B 250 FCircle Y1 position Parameter C fie FCircle radius Parameter D jo FCircle not used X Cancel Type can be text line empty rectangle filled rectangle circle cross X cross star ellipse disk filled ellipse Color 16 possible colors Width width of the symbol in screen points Parameters A B C and D depending of the feature to draw Text label free for the user file C ADHOCw HELP adw2d_o htm 5 of 6 15 02 02 09 34 23 Text and overlays Bold and or italic free for text To return to the coordinates press the swap to coord button Saving the coordinates and overlays Coordinates and overlays are saved in the ADC context file Don
33. 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 18 35 G01 0182 16 Batch Lower 18 19 55 G01 0182 16 Batch Lower 18 21 22 G01 0182 16 Batch Lower 18 22 46 G01 0182 16 Batch Lower 18 24 16 G01 0182 16 Batch Lower 18 25 46 G01 0182 16 Batch Lower 18 27 16 G01 0182 16 Batch Lower 18 28 46 G01 0182 16 Batch Lower 18 30 07 G01 0182 16 Batch Lower 18 31 24 G01 0182 16 Batch Lower 18 32 39 G01 0182 16 Batch Lower 18 33 57 G01 0182 16 Batch Lower 18 35 19 G01 0182 16 Batch Lower 18 36 39 G01 0182 16 Batch Lower 18 38 01 G01 0182 16 Batch Lower 18 39 30 G01 0182 16 Batch Lower 18 40 57 G01 PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHE
34. 1x1 C 2x2 C 4x4 C 8x8 C 16x16 X Cancel Help FITS CCD files this mode is used in Byurakan and can be easily adapted for other telescopes CCD Cigale acquisitions As for the IPCS 256x256 the program is able to wait and integrate real time acquisition The basing FITS files are 2D and contain the image of a channel One FITS file has a simple name Xnnncckk FIT or Xnnncckk FITS where X is a literal character B for Byurakan for instance nnn is the observation number from 000 to 999 ccis the cycle number or scan number 00 to 99 and kk is the channel number 00 to 99 The log file is Xnnn LOG Interlacing is connected to the sequence of observations In CCD mode the observer interlaces frequently the channels in order to minimize the effect of the variation of the transparency and the air mass Interlacing 2 gives a sequence 1 3 5 2 4 6 Interlacing 4 gives a sequence 1 5 9 3 7 11 2 6 10 4 8 12 ADw3D program manages the waiting of the channels in every case The dialog window appears as 08 ADw ADA format _ Of x ADHOCw Origin of the data cubes M Code of the observation gt 7 Cycles to integrate Indicate here one of the input data files Choose file Start cycle fi End cycle 3999 1060x514 FITS files Dimensions of the orginal image Dim X 1060 Dim Y 514 Nb channels 24 H Usually DimX 1060 and DimY 514 i Binning 5 1x1 2x2 C 424 C 8x8 C 16x16 ie Channel Interlacing no
35. 4 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns 20 00 30 00 40 00 50 00 60 00 70 00 80 00 90 00 When the array is validated the user must press the Read array and return to image button On the image menu if the Fixed parameters button is active computation and drawings will refer to fixed parameters If the Params r button is active array will 100 110 00 O be taken in account ADV crown sectors file The ADV sector Example 120 00 110 00 100 00 90 80 10 60 50 40 30 20 10 10 20 30 40 50 60 70 80 90 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 00 file is an ASCII file containing rmin is facultative of ADV file 110 00 15 00 55 00 2320 00 30 00 1 100 00 15 00 55 00 2320 00 30 00 2 30 00 40 00 50 00 60 00 70 00 80 00 90 00 100 00 110 00 120 00 24 00 27 00 30 00 33 00 36 00 15 00 15 00 15 00 15 00 15 00 rmax 64 00 67 00 70 00 73 00 76 00 55 00 55 00 55 00 55 00 55 00 PAmin PAmax 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 2320 00 30 00 30 00 30 00 30 00 30 00 30 00 30 00 30 00 30 00 30 00 Vs and Incli for every crown sector The format is free and the file can easily be edited 90 00 15 00 55 00 2320 00 30 00 3 80 TO 60 50 20 30 40 50 60 70 80
36. Store TV levels as custom values for acquisition Acquire frame Abo Crosses display Test PerotFabry with auxilliary TY display Gests 4210 Imbd 6662478 nhc 24 gt PPatep 29690 PFbase 356 286 E5700 serial interface COM channel PF value 100 o E hove PF file C ADHOCw HELP adwi_b htm 3 of 4 15 02 02 09 34 02 ADwIPCS tests The Discri Black level and White Level are critical The user can store the TV levels as custom values for acquisition i e transfer these values to the acquisition parameters Warning this is not automatical To move the channel the user can give the channel number or the hardware PF value they are directly connected Rounding is done Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwi_b htm Return to main ADHOCw menu Return to main ADwWIPCS menu file C ADHOCw HELP adwi_b htm 4 of 4 15 02 02 09 34 02 ADwIPCS THT ADwIPCS Return to main ADHOCw help Return to main ADWIPCS help THT and shutter management During the tests or duri
37. The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1oth htm Return to main ADHOCw menu Return to main ADwT1 menu file CI ADHOCW HELP adwT 1oth htm 4 of 4 15 02 02 09 34 30 ADwT1 user cubes ADwT1 Return to main ADHOCw help Return to main ADwT1 help C10 Creation of special user cubes This function allows to create special cubes by fixing the first channel reference and the spacing between channels The user can by this way create cubes with normalized spacing between channels 0 5 Angstroems 10 km s file C ADHOCw HELP adwt1c10 htm 1 of 4 15 02 02 09 34 30 ADwT1 user cubes ADw Create user cubes Pale Es ADHOCw Greaves af special user cules Input 3E file Ou tout 2B fil E Outut ADP parameter file defined with the output 3D fie m Pesenti O st chanel l ngstoems E560 00 Astchannellkm s Pano interfringe in Angtoems B65 itteingemkms 732 1 channelinAnguo ems 021 tchamelmkmes B5 a Output nb af channels 27 Assign wavelengths Angetraems 1st channel 6560 00 1 channel 10 21 Assign radial velocities kms Tet channel 130 05 1 channel 3 59 Note radial velocities are corrected trom heliocentric velocity Pa Execute Help x Abort Store maero s the output cube will have different dimensions the output cube will take place in a new directory as well as a new ADP parameter file
38. This file is adw2d_k1 htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_k1 htm 10 of 10 15 02 02 09 34 26 ADw2D kinematical functions user made crowns ADw2D Return to main ADHOCw help Return to main ADw2D help User made crown sectors and kinematical optimization The user can use self made crown sectors which have two advantages the crowns sectors can be not equidistant in radius there is the possibility to give different position angles PA p systemic velocities Vs p or inclination i p with respect to the distance to the center p in the plane of the sky In this case individual pixel velocities are computed as rotation velocities are Vrot x y Vrot p RV x y Vs p sin i p cos 6 radial velocities are RV directly coming from the 2D file 01 projected rotation is PR x y RV Vs p cos 8 Vs p The first operation is to define the crown sectors The all the displays and different operation on rotational velocities will use these crown sectors instead of the classical fixed kinematical parameters Then from these crown sectors the user can optimize within each crown sector the best major axis MA systemic velocity Vs and inclination i Not that global optimal PA Vs and inclination parameters can be easily obtained by defining very extended crowns in radius for instance 2 symmetric crown sectors with respect to the nucleus or 1
39. This file is adwt1_c2 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_c2 htm 3 of 3 15 02 02 09 34 51 ADwT1 menu CIGALE ADwT1 Return to main ADHOCw help Return to main ADwT1 help Cigale functions C AO aDwT1 Pytheas Z 10 x Hide task manager window Version Bring task manager to front A D H O Cw A DwT1 2001E JBx Obs Marseille 1280 s 1024 SE ppi General 2D 3D operations Cigale Profiles IPCS Tiger Pytheas Miscell Compute monochromatic continuum radial velocities line widths 2D maps ei Edit a batch file 4 Substract OH and or continuum from given areas pe Get photometric parameters from OH lines case of CCD gt ADX file iq Exec a batch file Get seeing analysis channel channel case of CCD gt ADS file Merging of several ADS seeing parameters files Photometric correction channel channel from seeing ADS file EA Show logbook Compute the calibration Finesse 7 Build custom made lambda cubes Ez Display control Get photometric parameters from rough analysis of non dephased channels Continuum substraction from given areas Execute a function Quit the program 7 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which c
40. To change the step or the threshold there are two ways click on the adequate button or fixed values or edit yourself the step or threshold field Then click on actualize full display Flip horizontally or vertically You can inverse the image in X or Y Visualization mode There are several possible modes square pixels means that the pixels can be easily recognize when the image is zoomed Smoothed pixels means that the pixel structure disappears when the image is zooms Isophotes are isocontours Square pixels isophotes superimposes both modes as well as Smoothed pixels isophotes Zoom area and pixel position value On the top of the screen the left image usually represents the 19x19 pixel zoom of the mouse position On the right the values of the XY position and the value of the pixel content are displayed You can change the cursor size default 1x1 pixel in this case the pixel content will be the mean value of all the pixels included in the enlarged cursor Whole image area On the top of the screen the right image usually represents the whole image Inside the white square indicates the frame of the displayed portion of the image You can move the displayed portion of the image by dragging the white square inside the whole image area Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to
41. Users manual ADHOCw Return to main ADHOCw help Printing your own copy of the User s Manual If you plan to work regularly with ADHOC it is an evidence that the paper User s Manual can help you a lot even if the totality of this manual is available on line during the execution of the programs Here is explained how to create your personal copy which is exactly similar to the printed User s Manual available at Marseille Observatory You will find all the components in the ADHOC HELP directory The operation is easy and takes less than half an hour The only thing is to print headers of the manual and of the different chapters from a small Word document ADHOCMAN DOC This document has only 13 pages 2 flyleaves 8 chapter pages and 3 for the tables of content It is suggested to print the 8 chapter pages on colored paper in order to separate clearly the different programs HTML files It is recommended to use Netscape or lEplorer which manage correctly the text The manual is about 350 pages Some pages must be printed in landscape format because they are full size images that cannot fit in a portrait format The ordering of the User s Manual is the following gt page 1 of adhocman doc gt page 2 of adhocman doc adhoc doc gt page 3 of adhocman doc 1 ADHOCw generalities coloured paper if possible adhocw htm adwworld htm adw_what htm adw_scr htm adw_inst htm adw_man htm gt page 4 of adhocman doc 2 Redu
42. copy to 2D image 1 button Copy to 2D image 1 pressing this button changes the image 1 If several images are displayed only the image 1 is changed This modification is only in memory To change also the disk file the user must then press the Save modified 2D file 1 button which appears as soon as the image memory if modified Undo 2D successive modifications this is the way to undo previous modifications Up to 10000 modifications can be recorded and retrieved in case of error Draw RV tics on profile is only used for profiles drawing on the 2D image If this box is checked a small tic appears at the top of all the profiles indicating the location of the measure of the 2D file 1 in terms of radial velocity The tic is normalized in modulo in order to appear always between the channel 1 and the last channel Modify replace and store profiles pressing this button let the following window appears file C ADHOCw HELP adw2d_e htm 5 of 8 15 02 02 09 33 54 ADw2D 3D profiles 20 ADw2D profile Channel 2 Original value 51 76 Modified value 51 76 Graph channel limits fi to 27 M FullY scale Graph mini 42 83 Graph maxi 64 34 Redraw with parameters above Store 1D profile RY to AD1 file Print window Store 1D profile lambda to AD1 file Save graph to BMP file Store 1D profile channels to 4D1 file Return quit graph Modifying dynamically the profile wi
43. don t change the values and go back to the acquisition task Print this window button allows to print the parameters as they are shown on the parameters window Tests Matrox PF button leads to the tests programs control and TV level adjustments control and moving of the Perot Fabry interferometer If you press on OK and the comment is not written and the prefix is not Test the following error occurs AD ADwIPCS warning Integrate file C ADHOCw HELP adwi_a htm 6 of 7 15 02 02 09 34 00 ADwIPCS Parameters Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwi_a htm Return to main ADHOCw menu Return to main ADwIPCS menu file C ADHOCw HELP adwi_a htm 7 of 7 15 02 02 09 34 00 ADwIPCS parameters full size ADHOCw photon counting task Version 21 04 2000 JBx show command ADHOCw photon counting acquisition parameters Identification of the observation cs El Prefix ic E Test Comment UCR RT RUE L 08 1 T ftest pretix is not incrementing i Type of acquisition
44. dump and batchs ADwFT Return to main ADHOCw help Return to main ADWFT help Dumps files content modifications You can display and modify manually the content of a 2D of 3D file EO ADwFT OF x Window scale aJ 10 ADHOCW File Translator sersion1 00 JBx pois Presentation 3D gt 3D 2D gt 2D 3D gt 2D slices 2D slices gt 3D File parameters Dump and modify Macros Function This function gives the possibility to dump and print the values of a full line of a 2D file or of the pixel spectrum of a 3D file Open file Values File name D Softuare FITSVIEN Ngcl3l o fit lt Ngc1 316o fit Line 100 l 1l 5 P 5 Dimensions I 512 ly 512 3 10 4 10 5 10 Coordinates of the value E 10 Line 7 15 8 15 fi 00 9 15 10 15 ne x B Print values Modify values Possible normalization of conversions new_value 4 old_value B A 1 0 B 0 0 About Help XM Quit File Translator Note than you must first indicate the line for 2D files or the coordinates of the pixel 3D files and then press on the Get values button file C ADHOCw HELP adwft_c htm 1 of 2 15 02 02 09 34 09 ADwFT dump and batchs You can then modify manually the values inside the displaying window and validate the change by pressing on the Modify values button Comment or information boulesteix observatoire cnrs mrs fr
45. existing additional n 1 channel will recover the channel 1 All the operations consider that the spectrum can be overlapped with a modulo n Open an existing ADHOCw parameters file ADP The user can open an already existing ADP parameter file The ADP file can be changed at every moment by using the A01 function of the ADwT1 program Create a new ADHOCw parameters file ADP The user create a new ADP parameter file When created the ADP file can be changed at every moment by using the A01 function of the ADwT1 program Execute create modify a global macro batch ADB command file This is the possibility to run global batches on successive directories These batch files are named ADB macro batch files and can be edited and run from ADwT1 This is the way to chain successive ADM macro files located in different directories and referring to different ADP parameters files A whole night of automatic work One object one directory one ADM macro file Several objects different directories several ADM files one unique ADB macro batch file file C ADHOCw HELP adwt1_ge htm 2 of 3 15 02 02 09 33 46 ADwT1_gene Global macro batch procedure Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IE
46. f30 dea foo faoo epoch 2000 Scale 1 screen pixel 1 000 arcsec This scale is for 512 screen pix Text coordinates parameters Text color Text size Text bold Yellow 20 Yes Vertical label space 2 0 00 Horizontal label space 0 min 10 00 sec Tics amp frame Vertical large tic space ine me asides x fo i 60 00 Tics color ly ellow gt Vertical small tic space J o pool Tics thickness 2 8 mm S N 7 9 LU T U Horizontal large tic space Frame bkad color Black rl lo min 10 00 sec Frame square yes rl Horizontal small tic space Frame color Yellow 0 minf2 00 me is Frame thickness 2 Y M Legend Color Lime 7 Text size 30 rl Bold yes Text lrregular galaxy To add text or drawing overlays click on Swap to overlays 12h 00m 10s 12h 00m 1ih 59m 50s alpha 2000 Export to Clipboard Kar Swap to overlays I f Export display to BMP Print _ AH Actualize tul display _ rreg U a r ga axy gt Save ADE context 7 Help Return to main Text coordinates can be pixels alpha delta or arcmin file C ADHOCw HELP adw2d_o htm 2 of 6 15 02 02 09 34 23 Text and overlays Center of the coordinates is defined by X and Y position in screen coordinates the screen size being 1 512 Use the running coordinates on the top right of the image to get the good center Center cross can be non cross or X cross Center cro
47. fadp new ADP parameters file in a different directory ss fpytheas binary file to transmit to G01 function fvrerif2 output verification calibration 3D file f file C ADHOCw HELP adwt1_f2 htm 6 of 8 15 02 02 09 34 33 ADwT1 TIGER 2 Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0134 16 Batch Lower 16 24 18 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER_CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 19 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 1
48. or barycenter the barycenter is computed above if emission or below absorption the level defined by the Y mouse position and inside the line defined by the X position Profile in large window the user can enlarge the profile measure in detail lines and zoom details Press here for more information Clear selection pressing this button deselects all previously selected cells Direct sets mode to direct pointing Barycenter sets mode to barycenter pointing The X position of the mouse indicates the line the Y position the lower if emission or upper if absorption level of computation Il this case a white tic indicates on the top where the measure was computed Absorption this box must be free for emission mode and must be checked for absorption mode file C ADHOCw HELP adwa2d_e htm 4 of 8 15 02 02 09 33 54 ADw2D 3D profiles Interfringe the user can choose a value to correct the wavelength and radial velocity values of the modulo of several interfringes positive or negative Chop a value to modify later pressing the left mouse button when inside the profile freezes the current value in order to record it later to the 2D image file Current color and chopped colors corresponding to the current and chopped values are displayed in 2 small rectangles in order to compare to the displayed image The chopped radial velocity RV is also indicated The 2D image can be modified with these values by pressing the
49. seeing 1 595770 pixels 0210 O1 Lower 09 23 20 Channel 26 dx 0 956918 dy 1 395879 seeing 1 595770 pixels 0210 O1 Lower 09 23 20 Channel 27 dx 0 950780 dy 0 596855 seeing 1 595770 pixels 0210 01 Lower 09 23 20 Saving control curves into BMP file 0210 01 Lower 09 23 21 Control graphic is buffered and can be displayed by pressing on the Display control button Display control The BMP graphic control file can be displayed during the data reduction or later BMP file During the data reduction the user can display or print the graphic in the display control window The BMP graphic looks like this file C ADHOCw HELP adwt1_c6 htm 4 of 7 15 02 02 09 34 48 ADwT1 seeing analysis SEEING 22 01 1999 09 23 20 displacements toplime fall scale 6 1966 pis YY displacements center aqual i full scale 6 1966 pix Seeing variations bottom red full scales 2 5231 pis The output ADS file gives the delta X and delta Y to correct in pixels plus the seeing in pixels and the channel number Note that the delta X and delta Y are here the correction to apply i e the inverse of the values given in the logbook which are the displacement By this way the ADS file can immediately be used to shift the image with the appropriate function C08 for instance Its content is like this 1 3243 0 7604L 2 285668 1 file C ADHOCw HELP adwt1_c 6 htm 5 of 7 15 02 02 09 34 48 ADWwT1 see
50. 1 enforced 1 mode_e force ellips to 1 if CCD 0 normal 1 enforced 0 0000 min_a min angle for phase 360 0000 max_a max angle for phase 0 0000 min_r min radius for phase 99999 0000 max_r max radius for phase 0 alpha hours 0 alpha minutes 0 0000000 alpha seconds 0 delta degrees 0 delta minutes 0 0000000 alpha seconds 0 0000000 reference year 0 0000000 time minutes 0 time hours 0 time day 0 time month 0 time year 0 0 0 0 0 0 0 0 0 0 1 dummy dummy dummy dummy dummy 0000000 dummy 0000000 dummy 0000000 dummy 0000000 dummy 0000000 dummy 83 numcom last command number executed Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in file C ADHOCw HELP adwt1_ad htm 4 of 5 15 02 02 09 34 20 ADwT1 ADP parameter files the adhocw help adhocw htm file This file is adwt1_ad htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_ad htm 5 of 5 15 02 02 09 34 20 ADwT 1 Channels tabulation ADwT1 Return to main ADHOCw help Return to main ADwT1 menu A02 Tabulate wavelength and r
51. 13 49 084457 0181 01 Lower 11 08 09 k tabz_ref 14 54 439568 0181 01 Lower 11 08 09 k tabz_ref 15 56 555294 0181 01 Lower 11 08 09 k tabz_ref 16 52 874104 0181 01 Lower 11 08 09 k tabz_ref 17 45 846287 0181 01 Lower 11 08 09 k tabz_ref 18 41 206387 0181 01 Lower 11 08 09 k tabz_ref 19 39 592953 0181 01 Lower 11 08 09 k tabz_ref 20 39 426067 0181 01 Lower 11 08 09 k tabz_ref 21 39 424767 file C ADHOCw HELP adwt1_c5 htm 7 of 11 15 02 02 09 34 46 ADwT1 photometry from OH file C ADHOCw HELP adwt1_c5 htm 8 of 11 15 02 02 09 34 46 0181 01 Lower 2 08 09 k tabz ref 22 39 811321 0181 01 Lower 08 09 k tabz_ref 23 39 908306 0181 01 Lower 2 08 09 k tabz ref 24 40 136875 0181 01 Lower 08 09 k tabz_ref 25 40 862461 0181 01 Lower 2 08 09 k tabz ref 26 41 045628 0181 01 Lower 2 08 09 measured a real b 0181 01 Lower 2 08 09 Analyzing channel 1 0181 01 Lower 2 08 09 a 0 981483 b 13 711790 0181 01 Lower 2 08 09 Analyzing channel 2 0181 01 Lower 2 08 10 a 0 863178 b 6 868777
52. 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 measured spectra 968 0182 16 Batch Lower 18 52 27 G01 PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info Comment or information boulesteix observatoire cnrs mrs fr Computing line 33 53 Computing line 34 53 Computing line 35 53 Computing line 36 53 Computing line 37 53 Computing line 38 53 Computing line 39 53 Computing line 40 53 Computing line 41 53 Computing line 42 53 Computing line 43 53 Computing line 44 53 Computing line 45 53 Computing line 46 53 Computing line 47 53 Computing line 48 53 Computing line 49 53 Computing line 50 53 Computing line 51 53 Computing line 52 53 Computing line 53 53 Nb total of object Correct end Note all ADHOCw help is in HTML The present HTML
53. 21 ADw3D wavelength maps Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_g htm 2 of 2 15 02 02 09 34 21 ADw3D mono cont RV ADw3D Return to main ADHOCw help Return to main ADw3D help Getting monochromatic continuum and radial velocities maps This function is available in the mono cont RV folder This folder is enabled only if the parabolic phase map is loaded and the wavelength cube is computed file C ADHOCw HELP adw3d_h htm 1 of 4 15 02 02 09 34 22 ADw3D mono cont RV Displayed 2D image 3 types of maps can be displayed with the same zoom but individual levels and palettes monochromatic emission continuum and radial velocities Note that these maps are only rough i e the computation is optimized to win computing time because this function is mainly useful for photon counting real time observations for which the processor power must let available for centroiding operations So no sorting or deconvolution operation is used Monochromatic computation the result is the maximum value mean value of the spectrum Continuum computation the result is mean value maximum value number of channels Radial velocity computation the result is computed on the maximum position and its two adjacent channels The radial velocity map can be displayed with a mask in order to get only the velocities of the most intense monochromatic emission pixels This
54. 5 of 6 15 02 02 09 34 24 ADw2D kinematical functions the user presses on the shift key the points are drawn as 4 pixels in order to increase the visibility of the graph on old screens More zoom gives access to a more complex window in which the user can better manage the graph superimpose polynomial curves and run additional functions This button gives access to a new window the full kinematical graph window Double cursor and mouse displacements inside the selection sectors of the 2D image when the mouse is moving on the 2D image in a selected sector a double cursor identifies the exact point drawn in the velocities graph Params r gives access to the possibility to define non linear crows as user made crown sectors and kinematical parameters optimization Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_k htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adwa2d_k htm 6 of 6 15 02 02 09 34 24 ADw2D kinematical functions full graph ADw2D Return to main ADHOCw help
55. 55 0 55 0 Minimized Vs 1000 0 300 Miniized 30 0 Baise After computation the user can check graphically the results selecting individual crown sectors and pressing the get detail for crown number or Previous or Next buttons The resulting array can be saved as a TXT file by pressing the Save results into TXT file button The output TXT file is like that ADHOCw ADW2D crowns kinematical optimization Optimization parameters Xe from 119 0 to 119 0 by step 1 0 YE Erom 129 0 to 129 0 by step 1 0 PA from 20 0 ta 70 0 by step 2 0 Vs from 1000 0 to 1000 0 by step 1 0 Inci from 30 0 to 30 0 by step 1 0 Se crown parameters OPTIMIZATION n EI E2 PA1 PA2 Vs i nbpts XG ye MA Vs i sig vrot T 100 0 80 0 35 0 7520 1000 0 30 0 1264 120 0 130 0 54 2 1000420 30 0 3 10495 95 3536 2 80 0 60 0 35 0 75 0 L10000 30 0 978 120 0 130 0 54 2 1000 0 30 0 3 49116 84 142 3 60 20 40 0 35 0 7520 100070 300 694 120 0 130 0 56 2 1000 0 30 0 4 075 71 2822 4 lt 40 0 20 0 35 0 7520 1000 0 30 0 419 120 0 130 0 56 2 1000 0 30 0 5 22381 55 7213 Bu 20 0 0 0 35 0 75 0 1000 0 30 0 138 120 0 130 0 56 2 1000 0 30 0 7 24018 35 9306 6 0 0 2030 35 20 750 L000 0 30 0 140 120 0 130 0 54 2 T0000 300 7 26597 36 0593 7 20 0 40 0 35 0 75 0 1000 0 30 0 419 120 0 130 0 54 2 1000 0 30 0 5 19757 55 8124 8 40 0 60 0 35 0 75 0 1000 0 30 0 694 120 0 130 0 54 2 1000 0 30 0 4 06702 71 3239 9 60 0 30 0 35 10
56. 60 50 41 31 TLs 12 16 25 35 44 54 64 SE 83 92 102 111 121 Angstroems 0 00 21 42 63 84 05 25 46 67 88 09 30 51 12 93 14 30 55 76 97 18 39 60 81 02 29 44 0 00 45 90 33 79 24 69 12 6565 6565 6566 6566 6566 6566 6566 6567 6567 6567 6567 6567 6568 6568 6568 6568 6568 6569 6569 6569 6569 6570 6570 6570 6570 6570 6571 km s 130 9 140 4 150 0 159 5 169 1 178 6 188 2 LPT 57 207 3 02 48 93 36 81 74 28 83 40 95 50 05 62 16 FL 26 81 38 216 226 236 245 255 264 274 283 293 302 312 321 331 341 350 360 369 319 1 65 85 06 27 48 69 90 LT 32 53 74 95 ES 36 57 78 99 20 41 62 83 04 25 45 66 87 08 1 3 3 SRE 2 4 9 4 4 4 9 4 3 4 8 4 5 4 90 45 00 54 11 66 21 76 33 88 42 VA 52 09 64 18 73 28 65 71 6571 6571 6571 6572 6572 6572 65 72 6572 657 657 657 657 657 657 657 657 657 657 657 657 657 657 657 657 657 657 88 8 98 4 07 9 17 4 27 0 36 6 46 1 Doel 65 2 474 484 493 503 OS 522 932 541 551 560 570 lO 589 598 608 618 627 637 2 5 7 9 a 3 5 q 9 52 3 3 3 4 4 4 4 4 Ds Ds 5 5 Ds 6 6 6 6 2 5 0 5 9 6 1 6 1 6 83 37 92 47 04 59 13 68 23 80 35 90 44 99 56 11 66 21
57. 646192 Zone 1 857755 Zone 1 056425 Zone 1 109934 Zone 1 996847 Zone 1 715267 Zone 1 504380 Zone 1 452300 Zone 1 443784 Zone 1 438739 Zone 1 444460 Zone 1 449481 Zone 1 459768 Zone 1 472471 Zone 1 000000 Zone 1 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_c htm Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_c htm 3 of 3 15 02 02 09 33 57 ADw3D 3D display module ADw3D ADHOCw program to display 3D files Return to main ADHOCw help ADHOCw 3D display Bie E3 ADHOCw 3D display from real time acquisition OR already acquired data J Boulesteix ADHOC cubes AD3 or _DA3 files From chennel chennel observation acuisition slices C IPCS real time or deferred acquisition 256x256 Thomson detector 2 bytes coordinate ADA files ADHOCw Szex Size Framerecord C IPCS real time or deferred acquisition ICCD 4 or 6 bytes coordinate ADA files 512 st 2 No x Deferred acquisition from 6m telescope recorded pho
58. 7520 LOCO 0 30 10 978 120 0 130 0 54 2 1000 0 3040 3 48631 84 1665 LO 80 0 100 0 35 0 75 0 1000 0 30 0 1259 120 0 130 0 54 2 1000 0 30 0 3 0985 95 363 file C ADHOCw HELP adw2d_k2 htm 11 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns Mean results weighted with nb of points Xc center 120 00 pixels Yc center 130 00 pixels Major axis MA 54 36 degrees Systemic velocity Vs 1000 00 km s Plane inclination i 30 00 degrees Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_k2 htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_k2 htm 12 of 12 15 02 02 09 34 27 ADw2D ADw2D_kin full size AB ADHOCw 20 Ix 1256 ly 1256 lz J1 B Mouse arga 1 Gaso zoom 19x19 pix ipi 1 txt px EF Export display to BMP j 5 Setup printer BP Print Save ADC context Ha x Quit the program Mouse arga 2 hd vr Whole image Parameters Image Mini 2199 Max 2451 Display parameters T Flip vertivally T
59. 8 15 02 02 09 34 33 ADwT1 TIGER 2 Output 3D wavelength file as the output cube will have different dimensions the output cube will take place in a new directory as well as a new ADP parameter file In this case a special window creating output cubes with different dimensions will appear Output ADP parameter file this file will be created in the same directory than the output 3D wavelength file Output eventual PYTHEAS coefficients this is a binary file create in the input directory which is used to transmit to the G01 function all the information on the spectra position dispersion Output verification calibration cube this file will be created in the same directory than the output 3D wavelength file It allows to the user to measure the calibration and check that all the output pixels are correctly calibrated This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example oo ee fcalib D Pytheas SH152 sum_P039 ad2 fpos D Pytheas SH152 TIGER_pos TXT fwl D Pytheas SH152 TIGER_wl tmp fverif D Pytheas SH152 TIGER_measured_calib AD2 fin D Pytheas SH152 sum P038 ad2 threshold 3450 height 0 mode 1 degree 1 x1 0 x2 20 sigma 3 xc 500 000 yc 250 000 wlref 6562 780 mode _ ref 1 space 20 00000 angle 0 000 x11 6520 0
60. ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_b htm file C ADHOCw HELP adwa2d_b htm 2 of 3 15 02 02 09 33 48 ADw2D main display screen Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_b htm 3 of 3 15 02 02 09 33 48 ADw2D ADw2D_b full size 2D small a BSS 4 Ix 1512 N oit C b 512 le o i 2 Save ADC context Help XM Quit the program 7 207 Mouse area 1 Cursor Mouse arga 2 zoom 19x19 pix 7 fist pix z Whole image x Parameters Image F file C ADHOCw HELP ADw2D_bt htm 15 02 02 09 33 49 r Display paremeters P Flip vertivally Image ar fh 28x128 z x0 Yo fist 207 Visualization mode Smoothed pixel 7 Flip horizontally r Action of the left button of the mouse Cross sections Integration of profile C Image modification C TE OVEnay Rainbow 7 C Kinematics Glaalevies wt FC Hisiadratns Seale mak id Minis 163840 000000axi 1035 000000 200 M Cross section parameters i 01 01 Thickness jo pixels ACA 10 10 100 100 1000 1000 200 Scale overlap Scale min Actualize full display ADw2D
61. ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1h10 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1h10 htm 3 of 3 15 02 02 09 35 04 ADHOCw new in the last versions ADHOCw What is really new in the last versions Return to main ADHOCw help Here are new functions of the last versions Click on the theme to get a full description Look also to the history txt file for minor modifications and corrections of bugs ADHOCw Version 2001F manages totally PYTHEAS data reduction Version 2001G 21 sep 2001 Correcting minor bugs Version 2001F 01 sep 2001 adwt1 new functions full TIGER data reduction F01 F02 adwt1 new functions full PYTHEAS data reduction G01 adw2d new possibility Zoom and measure in detail selected profiles Version 2001E 20 may 2001 adw 2d adw3d additional user defined color palette adw2d new possibility coordinates and user overlays text drawings to the image adw2d new possibility equidistant crowns in rotational curves adw2d new possibility choice of fonts colors and sizes in the rotational curve graph file C ADHOCw HELP adw_new htm 1 of 3 15 02 02 09 35 04 ADHOCw new in the last versions
62. Actions Valeur par d faut Nouveau Supprimer F Conime louverture apr s le t l chargement F Permettre l aper u rapide T Toujours afficher l extension BK _ Annuler Op ration de modification pour le type ADHOC Z Action Application utilis e pour effectuer action ae ID WADHO Cw adwed exe T Parcourir Utiliser DDE For ADC then give the ADC icon press Changer d ic ne Change icon and choose ADHOCw ICO which is distributed in the same directory that the executable programs file C ADHOCw HELP adw_ass htm 4 of 6 15 02 02 09 35 05 ADw2D 2D display module AD3 extension Modification d un type de fichier Description du type AD HOC 30 cube Tepe de contenu MIME Extension par d faut pour type de contenu F Achons Nouveau Modifier Supprimer Valeur par d faut M Confirmer l ouverture apres le telechargement CIE Annaler Op ration de modification pour le type ADHOC 3 D Permettre l aper u rapide l Toujours afficher l extension DADHOCwMAdwad exe ZT Utiliser DDE FIT or FITS extensions 2D FITS files can be open the same way Take example of the AD2 extension procedure file C ADHOCw HELP adw_ass htm 5 of 6 15 02 02 09 35 05 ADw2D 2D display module Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The
63. C Angstrocms g pit other Cali nat in fim 6390 953 Ahjel line R62 T00 20 including mask ER Store macro Calibration scan 6593 953 Object scan 6514 64 Ki f xij Help object RU am Helloc RY correct nn o fs y raz J Enceutc ts Fite ulify ihes pa ri ES CES T Mim ee ama exei mash x Ahmi This is one of the most critic operation of the Cigale data reducing because it is the base of the quality of the metrology On the file section the program propose you to create 4 x 2D files You can change their name if you wish file C ADHOCw HELP adwt1_c1 htm 1 of 6 15 02 02 09 34 17 ADwT1 phase computation The rough phase gives you the rough measurement of the calibration channel It is only a test file that you can display but it is not used in the further treatment The values stored in the rough phase are in channels The parabolic phase is the phase used by other functions it is the phase map This is one of the most important files of the CIGALE treatment Note that in order to be compatible with the old ADHOC software you can build back an old ADHOC DOS phase file from this parabolic phase by running the H02 function The values stored in the parabolic phase are in channels The sum of the calibration channels is explicit If the scanning was good this file must represent a uniform image only affected by the filter transmission and the quality of the optics of the calibration The Radial Velo
64. CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info file C ADHOCw HELP adwt1_g1 htm 7 of 14 15 02 02 09 34 36 microlenses 1 50 547 microlenses 51 100 547 microlenses 101 150 microlenses 151 200 microlenses 201 250 microlenses 251 300 microlenses 301 350 microlenses 351 400 microlenses 401 450 microlenses 451 500 microlenses 501 547 Number of the most calibration line 6598 953 calibration line 6532 882 Computing interference order 578 deviation order 579 deviation order 580 deviation order 581 deviation order 582 deviation order 583 deviation ADwT1 PYTHEAS 1 0182 16 Batch Lower 18 16 28 G01 5 354 channels 0182 16 Batch Lower 18 16 28 G01 5 030 channels 0182 16 Batch Lower 18 16 28 G01 4 706 channels 0182 16 Batch Lower 18 16 28 G01 4 382 channels 0182 16 Batch Lower 18 16 28 G01 4 059 channels 0182 16 Batch Lower 18 16 28 G01 3 735 channels 0182 16 Batch Lower 18 16 28 G01 3 411 channels 0182 16 Batch Lower 18 16 28 G01 3 088 channels 0182 16 Batch Lower 18 16 28 G01 2 764 channels
65. CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info file C ADHOCw HELP adwtt_g1 htm 9 of 14 15 02 02 09 34 36 order 605 order 606 order 607 order 608 order 609 order 610 order 611 order 612 order 613 order 614 order 615 order 616 order 617 order 618 order 619 order 620 order 621 order 622 order 623 order 624 order 625 order 626 deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation ADwT1 PYTHEAS 1 8 239 channels 0182 16 Batch Lower 18 16 28 G01 8 563 channels 0182 16 Batch Lower 18 16 28 G01 8 887 channels 0182 16 Batch Lower 18 16 28 G01 9 210 channels 0182 16 Batch Lower 18 16 28 G01 9 534 channels 0182 16 Batch Lower 18 16 28 G01 9 858 channels 0182 16 Batch Lower 18 16 28 G01 10 181 channels 0182 16 Batch Lower 18 16 28 G
66. Flip horizontally Graph area Rainbow Scale max 2360 Threshold 0 1 01 1 10 10 100 100 1000 1000 Visualization mode Square pixels 100 100 1000 1000 Scale mir 2200 Scale overlap I Actualize full display file C ADHOCw HELP adwad_kt htm 15 02 02 09 34 28 Action of the left button of the mouse C Cross sections Integration of profile C Image modification C Text overlay Kinematics of galaxies e Kinematics of galaxies Cor atare fr FIr Olr fe example adk Load file Save to file M automatic saving C Params fr Te Yc i 21 00 km s Fixed parameters Center of rotation Systemic velocity 13320 00 incli w r sky PA wir top 1 2 sector 30 00 35 00 f20 00 de P PAAITELESS EJES CROWNS crowns 4 pix Rmin f 128 0 pik Yimin Rmazj128 0 pix More zoom all 4 quadrants blue red 2120 0 km s Vmax 12520 0 km s f Redraw graph ADwT1 Global macro batch Return to main ADHOCw help Return to main ADwT1 help Global macro batch For global batch execution the user must first define a ADB global batch command file When running the Execute create modify a global macro batch ADB command file the ADwT1 program loads the ADWTO global batch monitor program This monitor allows the user to run batch files successively in different d
67. Help EB Save to BMP XM Quit the program lambelisg5 ad3 Y Ty I Multiple 30 cursors Value EJ Zoom 19x19 pixels Phase Sum or individual channels Interferograms Wavelength maps Mono cont AV Monochromatic continuum and RV mans RSR file C ADHOCw HELP adw3d_h htm 2 of 4 15 02 02 09 34 22 ADw3D mono cont RV Monochromatic continuum and RV maps Radial velocities gt re compute maps Display parameters Graph area For real time Photon Counting observations The monochromatic continuum and radial velocities maps are not computed continuously The observer must recompute maps regularly This operation is done in background task with the parameters Image area 204128 262128 indicated below x0 Yo jes 53 Displayed 2D image Zoom in rough monochromatic emission mouse right button C rough continuum oy Zoom ou shift mouse right button radial velocities from 3 channels IV RY display threshold 30 This threshold is in monochromatic map intensity units Rainbow Displayed profile in the top zoom box C interferograms rough pe wavelength maps dephased Computation parameters Perot Fabry characteristics p 791 at 6562 780 Angstroems Phase reference wavelength channel 1 e598 950 A Scanning wavelength Zero velocity wavelength 6562 780 6562 780 A Mean tadial velocity RY correction fex heliocentric 0 00 kms 0 00
68. In this case a special window creating output cubes with different dimensions will appear The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DAS This function can be execute directly by pressing the Execute button or in batch by file C ADHOCw HELP adwt1c10 htm 2 of 4 15 02 02 09 34 30 ADwT 1 user cubes pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example USER_CUBE fin E ADHOCws_ plus BLAISOUS lambda ad3 fout E ADHOCws_plus BLAISOUS bidoni toto ad3 fadp E ADHOCws_plus BLAISOUS bidonl truc adp nb_channels 20 lambdal 6562 78 delta_lambda 0 28 keyword content options USER CURE delta lambda spacing between 2 channels in the output data file in Angstroems Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1c10 htm 3 of 4 15 02 02 09 34 30 ADwT 1 user cubes Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printi
69. Lower 21 33 23 Coordinates 1 to be modified 241 000000 ref 171 000000 349 000000 0017 01 Lower 21 33 23 Coordinates 2 to be modified 355 000000 ref 361 000000 307 000000 0017 01 Lower 21 33 23 Mean squares 0017 01 Lower 21 33 23 gt angle degrees 330 0203 sigma 0 3364 ADwT1 rotation scaling XYZ translations 0017 Ol1 Lower 21 33 23 gt echelle 1 2460 sigma 0 0093 0017 O01 Lower 21 33 23 gt deltaX 19 1720 sigma 0 8051 0017 01 Lower 21 33 23 gt deltaY 150 9243 sigma 0 8190 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b11 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1b11 htm 4 of 4 15 02 02 09 34 43 ADwT1 sorting eliminating interpolating profiles ADwT1 Return to main ADHOCw help Return to main ADwT1 help B12 Sort eliminate interpolate profiles on sigma for 3D files This function is frequently used to suppress cosmic rays on CCD channels file C ADHOCw HELP adwt1b12 htm 1 of 5 15 02 02 09 34 44 ADwT1 s
70. MISCELLANEOUS H02 function Translation of a parabolic phase into an old ADHOC DOS phase H03 function Create a dummy homogeneous 2D or 3D file H04 function Instrument tuning using image sequences H05 function Various peculiar cube corrections H06 function Precessions and object visibility H07 function Sideral time clock H08 function Interference filters selection H09 function Perot Fabry etalons characteristics and Queensgate constants H10 function Common nebular and calibration wavelengths Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h htm 2 of 2 15 02 02 09 34 58 ADwT1 creation a dummy homogeneous file ADwT1 Return to main ADHOCw help Return to main ADwT1 help H03 Creation of a dummy homogeneous 2D or 3D file ADw fill dummy fles ADHOCw Creates of a fdummy fhomogeneaus 20 ar 20 tile f Create a 20 file Create a SD file Output the Value that will fil the file fo Set filli
71. OBJ AD3 gt OBJ1 AD3 Note that for cosmics it is better to eliminate on the derivatives A 3 and nb_iter 2 are good starting parameters 6 if necessary for CCDs clean the wrong columns or lines with the function B14 of the ADwT1 program OBJ1 AD3 gt OBJ2 AD3 7 Eventually only not recommended for beginners who will go directly to paragraph 8 for CCDs observations if the seeing conditions or the tracking displacements changed correct from seeing and displacements identify stars coordinates ADw2D program displaying the sum of all object channels compute seeing and displacement parameters for every selected star from the OBJ1 AD3 or OBJ2 AD3 cubes with the function C06 of the ADwT1 program OBJ AD3 gt SEEING n ADS All the created seeing files are of the ADS type check if this correction is really necessary for that compare the output BMP files from the computation of all the star positions If features are random don t correct you will simply add noise merge the ADS seeing parameters files of the different stars into one unique seeing parameters file function CO7 of the ADwT1 program correct the original not dephased file from the seeing function C08 of the ADwT1 program OBJ2 AD3 gt OBJ3 AD3 D Correct the clean cube from the CCDs photometrical variations along the exposure 8 the first operation is to identify the areas zones which are free from the object spectrum This can
72. Return to main ADw2D help Full kinematical graph window When pressing the more zoom key in the kinematical menu the user opens a new window ADHOCw ADw2D kinematics E i iojxj This is the legend d 2 32 Wir alt alt aptr quadrants 2 3in2 LE EC d define points 1 oe oo A je s 05 f100 0 Create 2D image from the curve Create 2D residuals from the care Save data to TXT Frame Symbols Digits Legend amp add BM a m Save graph as BMP fis3 00 121 00 bd FY pointe file C ADHOCw HELP adw2d_k1 htm 1 of 10 15 02 02 09 34 26 joo M pa ADw2D kinematical functions full graph opensa 2 filled square Me Mass distribution r RotV or RV current values are following the mouse location in the graph Print this window prints the total graph window Save graph as BMP saves the upper graph as a BMP graph file Help displays a help text relative to this window Redraw graph rereads parameters a re draws the graph Quit this window returns to the basic 2D window Selection parameters file C ADHOCw HELP adwa2d_k1 htm 2 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph Rotation velocities 2 1 CROWNS blue ed BRS 4 quadrants 2 3 in 2 Rotation velocities radial velocities projected rotation the user must choose here what to draw rotation velocities are Vrot p RV Vs sin i cos 6 radial velocit
73. Typical reduction procedure When you will run the ADwT1 program note that you must define first a dedicated sub directory There is only one observation in one dedicated sub directory This means that all the 2D and 3D files inside one directory have the same dimensions and the cubes or phase maps have the same wavelengths In fact there is only one ADP parameter file and only one ADL logbook file in one sub directory dedicated to one observation For example if you extract a portion of a cube function B10 the basic dimensions will change and it will be necessary to create another sub directory for the new files and create a new ADP parameter file 3 Possible typical procedure Suppose that you have one object cube OBJ AD3 and one calibration cube CAL AD3 A Get a look on the observation 1 check the sum of all object channels function BO1of the ADwT1 program OBJ AD3 gt SUM_OBJ AD2 and then visualize the 2D file with the ADw2D program Or use the ADW3D program also convenient for that Note that it is never necessary to exit from an ADHOCw program ADwT1 ADw2D ADw3D to work on the same files Simply launch a new executable from ADHOCW EXE Even several ADwT1 ADw2D or ADw3D can run at the same time B Get the phase map 2 check the calibration channels visualize the CAL AD3 file with the ADw3D program in order to check the correct scanning no special ring feature is expected from the sum 3 compute
74. Wahia of PU ADwT1 masking operations POSTIPS ULSI SA ab D Yee Ss r Ee SEC G CO masimu F3 F2 if F2 is inside 4 and B values F1 else F3 F2if F2is outside 4 and B values F1 else value of C Use an execution mask a Execute Help x Abort EX Store macro The program accepts 2D or 3D files it recognizes automatically the type of the input file The user has the following possibilities in which F1 and F2 represent two 2D or 3D input files F3 is the 2D or 3D output file F3 F3 F3 F3 F3 F3 F3 F3 else F3 else F3 F3 F3 F3 A F1 B A F1 F2 A F1 F2 maximum of minimum of null if F2 null if F2 F1 if F2 is F1 if F2 is F1 if F2 is F1 if F2 is F2 if F2 is F2 if F2 is F2 C B B F1 and F2 F1 and F2 null not taken is null value F1 else is null value F2 else inside A and B values null outside A and B values null inside A and B values F2 else outside A and B values F2 else inside A and B values F1 else outside A and B values F1 els The user must provide the names of the input and output files and the values of the floating variables A B and C It is possible to enforce the A or B values to minimum or null value 3 1E 38 or to maximum value 3 1E 38 If the result is less than 3 1E 38 the value is set to 31 E 38 null value If the result is more than 3 1E 38 the value is set to 3 1E 38 The input files can
75. a data file button you see the following window ADwFT File information The dimensions type and comment are displayed FITS header By pressing on the FITS header button if the file is of FITS format you see the following window file C ADHOCw HELP adwft_b htm 2 of 6 15 02 02 09 34 08 ADwFT files structure ADwFT FITS_header Efel X NAXISZ 512 EXTEND T Tables following main image BLOCKED T Tape may be blocked OBJECT NONE TELESCOP INSTRUME OBSERVER DATE OBS DATE MAP 24 03 94 BSCALE 00000000000E 00 REAL TAPE BSCALE BZERO BZERO 0 00000000000E 00 BUNIT EPOCH 0 000000000E 00 EPOCH OF RA DEC BLANK 32768 Blanked pixel tape value DATAMAX 1 037890381E 03 MAX PIXEL VALUE DATAMIN 5 450683594E 00 MIN PIXEL VALUE CTYPEL RA SIN CRVALL 5 01966661513E 01 x Print FITS header Minimum and maximum By pressing on the mini and maxi button you see the following window file C ADHOCw HELP adwft_b htm 3 of 6 15 02 02 09 34 08 ADwFT files structure ADwFT mini amp maxi ADHOCw parameters By pressing on the ADHOCw parameters button if the file is of ADHOCw format you see the following window file C ADHOCw HELP adwft_b htm 4 of 6 15 02 02 09 34 08 ADwFT files structure oe ADwFT ADW parameters Pale Es General parameters of ADHOCw data files Modify if ne
76. accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b14 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1b14 htm 4 of 4 15 02 02 09 34 45 ADwT1 Photometric corrrection ADwT1 Return to main ADHOCw help Return to main ADwT1 help B15 Photometric correction channel per channel 8 ADw photometric correction ADHOCW Photemetic correction channelichame laput 30 file Input SE file containing channel photometric parameters Output 3D file T Use an execution mask 7 Help X Abort ES Store macro This function is applying a linear correction to a 3D file new_value a old_value b The a and b values different for every channel are read from a ADX file This function is used frequently to correct the CCD observations from the photometric fluctuations see examples in the CCD procedures and also the C05 function The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD3 file C ADHOCw HELP adwt1b15 htm 1 of 4 15 02 02 09 34 45 ADwT1 Photometric corrrection This function can use an execution mask When the execution mask doesn t allow the operation the extracting value is s
77. acquire and display a single 2D image In this case nevertheless the structure of the 3D files is maintained apparently channels are scanned in order to allow a similar display every second So the total 2D exposure time will be a function of the pseudo number of channels the pseudo exposure time per channel the pseudo number of cycles taking in account starting channels and cycles But all these pseudo channels images will be of course superimposed 3D calibration initializes the default calibration scanning parameters 3D object initializes the default object scanning parameters Type of source TV IPCS integrates the direct photon counting TV Random simulation is a test of simulated photons The appearing box named random number of points indicates the number of simulated photons per frame of 1 25 second Scanning parameters Nb of channels forced to 50 for 2D image Note that if the number of channels is superior to 99 the user must request the appropriate Data file names parameters which is no more the default value Exposure time per channel This value in seconds is treated as an integer impossible to scan times which are fraction of seconds Maximum number of cycles Note that if the number of cycles is superior to 99 the user must request the appropriate Data file names parameters which is no more the default value Starting channel number the observer can decide not to begin at ch
78. adhocw help adhocw htm file This file is adwtic11 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1c1 1 htm 8 of 8 15 02 02 09 34 53 ADwT1 Photometric corrrection ADwT1 Return to main ADHOCw help Return to main ADwT1 help B17 2D or 3D mosaic This function allows to build mosaics First create a directory and a null file function HO3 of the final dimensions Then you can replace or add any file of different dimensions Replace means that the value of the added file replaces the original one Superimpose means that there is a combination of original and added values Transparent value means that if the added file contains this value no operation is done Virtual pixel position is in final frame and represents the displacements M B17 ADw mosaic Ee 10 x ADHOCW Mesas B17 Input 2D or 3D file original mosaic Choose file Input 2D or 3D file to add Choose file Dimension of the subfile CE x Y Z Virtual pixel at mosaic position 1 1 X Sa Y Ouput 2D or 3D file final mosaic Choose file C Replace A 0 3 Superimpose Pee B 0 7 Result A mosaic in if no overlap Result B mosaic in B if no overlap final origin 2000 Result A mosaic B added 2 if overlap 715 final 1400 Result mosaic if overlap and added transparent file C ADHOCw HELP adwt1b17 htm 1 of 3 15 02 02 09 34 54 ADwT1 Photometric
79. and ADw3D user palette ADHOCw Return to main ADHOCw help User color palette for ADw2D and ADw3D It not obvious to represent correctly colors on viewgraphs or paper For that a user palette has been added to ADw2D and ADw3D palettes In ADw2D and ADwsbD the palette can be now rainbow black and white black and white inversed color1 color2 color3 or user 16 colors Compared to other palettes user 14 color differs from two points the palette is only 16 colors instead of 256 but the 16 colors are distributed along the same levels as for 256 colors the colors of the palette can be changed by the user To change colors simply select the palette user 16 colors The following window appears every time the palette is selected The user can let it unchanged or change colors file C ADHOCw HELP adw_uspa htm 1 of 3 15 02 02 09 33 50 ADw2D and ADw3D user palette AD ADw2D User color palette O x ADw2D definition of the user 16 colors palette Click on a color to change it The current user palette is saved continuously in a system file This palette will be reload automatically when executng ADw2D Use the load and save functions to transfer the palette onto another computer To access again to this color configuration menu it is necessary to select again the User 16 color palette from the palette box Pressing simply Actualize full display redraws the
80. and let the user to modify it with the mouse This option is extremely useful when the object emission and the OH emission are present everywhere in the field The user can by this way build his own profile rejecting the object contribution file C ADHOCw HELP adwt1_c4 htm 2 of 6 15 02 02 09 34 15 ADwT1 OH and or continuum substraction 2 Detail profile MX During the computation the following BMP file is generated and can be displayed in real time in the display control window It is then stored as indicated in the Output control BMP file indicated by the user in the menu file CI ADHOCW HELP adwt1_c4 htm 3 of 6 15 02 02 09 34 15 ADwT1 OH and or continuum substraction OH substraction 24 03 1993 10 17 31 Origin yellow Mini 4 883E 05 Maxi 7197E 05 Amplitude 2313E 05 per pixel Final red Mini 0 01194 Maxi 001056 Amplitude 002251 per pixel This function can use an execution mask When the execution mask doesn t allow the operation the cube value remains unchanged This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example nt fin Jbx_portable D ADHOCWS_plus BLAISOUS Imbd_brut ad3 fout Jbx_portable D ADHOCWs_plus BLAISOUS lmbd_org AD3 fzones Jbx_portable D ADHO
81. are predefined patterns values are displayed on the right Smooth Smooth Blur Sharpen Detail Edge enhance Edge enhance User smoothing mode is a pattern which is pre defined by the user and can be simply loaded from an ASCII file special ASCII format The user can edit any of the patterns even the predefined ones and store them as user patterns in ASCII code in order to use them later as user smoothing patterns The user must define the names of the 3D input and output files The null values are not taken in account in this computation The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD3 This function can use an execution mask This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network User file containing filter values This optional file which can be stored by pressing the Save user values button retrieved by pressing the Load file C ADHOCw HELP adwt1_b8 htm 2 of 4 15 02 02 09 34 40 ADwT1 spectral smoothing user value button or edited with a common text editor is an ASCII file Its structure is the following H Spectral smoothing user file NN H H H H PRR O owe Es one i ous 102 i
82. be connected on the VGA plug of the Matrox Genesys board The programs which require this second display are marked with an asterisc but are not scratch because the possible absence of the second display This optional second screen display must manage 1024x766 pixels minimum Simple message on screen Continous TY acquisition Grab a single 768x576 image in 402 format Grab a single 5124512 image in AD2 format ite iti ns lt allows to TUNE TV Move Nail test the PF interferometer Tune THT Choose a function and execute Execute function x Returnto program Stop Tuncihion Simple message on screen checks that the MATROX board is working even if the TV synchronization is absent Continuous TV acquisition checks the TV acquisition Grab images allows to keep track of tests Grab images and identify photons is the base of the TV tuning See window below Move and test the PF interferometer to check the P rot Fabry see window below file C ADHOCw HELP adwi_b htm 2 of 4 15 02 02 09 34 02 ADwIPCS tests Fa ADHOCw Test grabing photon counting oix Wrarning You need an auxiliary TY monitor connected to the VGA plug of the MATROX board for these tests Test MATROX and centroiding with auxilliary TY display f TVIPCS Random simulation Discri i l Black iul 135 Ea White lul 150 E def 20 m a def 51 En def 245 relief unusual Tune THT
83. browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_new htm Return to main ADHOCw menu file C ADHOCw HELP adw_new htm 3 of 3 15 02 02 09 35 04 ADw2D 2D display module ADHOCw Return to main ADHOCw help Assigning file extensions to ADHOCw programs If the user assigns file extensions it is possible to click simply on the file icon in the Explorer to immediately display the 2D or 3D file s without any dialog DA2 AD3 and ADC extensions can be accessed Procedure In the Explorer system program open Affichage View or Display and Options then Types de fichiers Files types The procedure is similar for AD2 AD3 and ADC extensions AD2 and ADC run ADw2D exe AD3 run ADw3D exe Nevertheless for ADC it is necessary also to change the icon It is also suggested to do similar operations for FITS files AD2 extension file C ADHOCw HELP adw_ass htm 1 of 6 15 02 02 09 35 05 ADw2D 2D display module Options Affichage Types d fichiers Types de fichiers enregistr s E ace Image a Houveau Type ADHOC 20 conteste ti ADHOC 20 image __ Supprimer lis ADHOC 3D cube Modifier Ee Adobe ST able 3 0 fe Ado
84. browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_g2 htm file C ADHOCw HELP adwt1_g1 htm 13 of 14 15 02 02 09 34 36 ADwT1 PYTHEAS 1 Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_g1 htm 14 of 14 15 02 02 09 34 36 ADwT1 menu OPERATIONS 2D 3D ADwT1 Return to main ADHOCw help Return to main ADwT1 help 2D 3D operations functions B Bring task manager to front A D H O Cw A DwT1 Version 99A JBx Obs Marseille 1280 x 1024 96 ppi General 20 30 operations cigale Profiles IPCS Tiger Pytheas Miscen Extract a 2D channel from a 3D file insert a 2D channel into a 3D file Get minimum and maximum of a 2D or 3D file t EA Edit a batch file Arithmetic operations on a 2D or 3D file Fout f F1 g Exec a batch file B06 Arithmetic and masking operations between 2D or 3D files Fout f F1 F2 BO Arithmetic operations between a 3D file and a 2D file Fout3D f F3D F2D B08 Spectral smoothing on a 3D file A B09 Spatial smoothing on a 2D or 3D file Display control B10 Extraction of a sub cube 3D or a sub image 2D B11 Inversion Rotation scaling X
85. calibration mode _order interference order used 0 computed 1 approximated given by user file C ADHOCw HELP adwt1_g1 htm 5 of 14 15 02 02 09 34 36 ADwT1 PYTHEAS 1 integ x1 xl2 stepz wlref fout fadp fpytheas fverif fverif2 spot integration l0 no 1 yes starting wavelength Angstroems lending wavelength Angstroems wavelength step Angstroems reference object line output 3D file in a different directory new ADP parameters file in a different directory input binary file to transmitted by F02 function zero wavelength output 2D verification file zero wavelength output TXT verification file Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Opening and creating miscellaneous files 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Reserving arrays 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Reading ADH Pytheas file 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Mean height of the spectra 5 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Integration of the pupil spots width 3 pix height 5 pix 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Output cube dimensions 93 26 901 0182 16 Batch Lower 18 16 22 G01 P
86. carre elementaire TOUJOURS 1 ix1 TOUJOURS 1 ix2 dimension X iy1 TOUJOURS 1 ly2 dimension Y NC nombre de canaux ligne 2 xikms vr1 ckms clamb xlamb1 xilamb format libre ou xikms interfrange en km s a la lambda observee vri vitesse radiale du premier canal ckms km s par canal a la lambda observae clamb A par canal a la lambda observee xXlamb1 longueur d onde du premier canal file C ADHOCw HELP adw_what htm 9 of 15 15 02 02 09 33 45 ADw what is ADHOCw Xilamb interfrange en A a la lambda observee ligne 3 commentaire 78 caracteres maxi format a78 ligne 4 identification 5 car et nom objet 20 car format a5 5x a20 ligne 5 vitesse de correction au soleil format libre Cette cinquieme ligne ne sert si elle existe que pour VISU3 pour corriger le tic de la mesure en VR qui se positionne verticalement au dessus du profil trace Cette cinquieme ligne peut etre absente auquel cas il n y aura pas de decalage de tic dans VISUS3 3 EIC compressed format These formats are special and come from La Silla Survey or Mexico observations The are also common on Sun Unix data reduction software written by Etienne le Coarer Note that the begining of thses compressed files contains ASCII strings which indicate some precious information size of the image scanning wavelength identification of the object This information can be read easily from any
87. channel with a seeing lower than the maximum seeing allowed value will be changes spatially degraded and the channels with a seeing larger than the maximum seeing allowed value will remain unchanged In order to guide the user it is possible to scan all the seeing values channel per channel in an array which appears in the right part of the window Then the computation is the following for every pixel every channel is computed separately The adjacent pixels supposed to enter in the seeing image are searched and are multiplied by a gaussian factor in order to degrade the image up to the maximum seeing allowed value Suppose that this value is msa and that the seeing of the channel is sch the gaussian convolution is computed for a half maximum width hma sqrt msa 2 sch 2 Then the profile or every individual adjacent pixel is corrected from the difference of phase beween the new location and the old one in order to take in account the variation of phase beween adjacent points All the values are linearly interpolated from the spatial and spectral coordinates which explains the long computation If the user choose the option avoiding interpolations the computational time is reduced with a factor 2 minimum In this case the nearest integer values are taken for the pixel intensities and the rephased channels instead of the spatial and spectral linear interpolations By this way the original cube is perfectly corrected 1 from t
88. coordinate numbered from 1 maski_y1 lincluded area y1 corner coordinate numbered from 1 maski_x2 lincluded area x2 corner coordinate numbered from 1 wa maski_y2 lincluded area y2 corner coordinate numbered from 1 maske_x1 excluded area x1 corner coordinate numbered from 1 maske_y1 lexcluded area y1 corner coordinate numbered from 1 maske_x2 excluded area x2 corner coordinate numbered from 1 maske_y2 excluded area y2 corner coordinate numbered from 1 maskc_k1 lower included channels numbered from 1 maskc_k2 upper included channels numbered from 1 maskv_v1 lower selected value file C ADHOCw HELP adwt1_ma htm 2 of 3 15 02 02 09 34 16 ADwT1 execution mask maskv_v2 supperselectvalue maskf image mask file name with full path maskf_v1 mask file lower limit value maskf_v2 mask file upper limit value Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_m
89. corrrection Result mosaic if overlap and added transparent AC CS Transparent value 3 1E38 null value Help Abort ER Store macro Mosaic operations adding mode reference value to add resulting value value replacement V1 anyone V2 anyone V2 superimpose V1 anyone V2 V1 transparent superimpose V1 null V2 null null superimpose V1 null V2 not null V2 b nor transparent superimpose V1 not null V2 null Vita nor transparent superimpose V1 not null V2 not null V1 a V2 b 2 nor nor transparent transparent This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several processor users and can be located on other computers accessible on the network Macro definition Example MOSAIC finl G Observations Nancy 12nov2000 12 ad3 fin2 G Observations Nancy 12nov2000 16 ad3 fout G Observations Nancy 12nov2000 17 ad3 mode 1 a 0 887 b 0 113 c 3 1E 38 x0 1 y0 1 1x 512 ly 512 12z 64 keyword content options MOSAIC finl 2D or 3D origin input file name with whole path fin2 2D or 3D added file with whole path fout 2D or 3D output file name with whole path mode adding mode 0 replace 1 superimpose file C ADHOCw HELP adwt1b17 htm 2 of 3 15 02 02 09 34 54 ADwT1 Photometric corrrection a multiplying coefficient
90. crown is free Inclination with respect to sky plane this inclination angle given here in degrees is 0 if the galaxy is face on and 90 if the galaxy is edge on Center of rotation it is usually the center of rotation Floating values are accepted The center coordinates are ADw2D compatible numbered from 1 Systemic velocity this is the real velocity of the center coherent with the radial velocities values contained in the 2D file 01 Position angle with respect to bottom top this position angle given here in degrees is 0 if the PA points to the top of the file C ADHOCw HELP adw2d_k1 htm 3 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph 2D image 90 if the PA points to the left of the image 180 if the PA points to the bottom of the image and 270 if the PA points to the right of the image It is recommended to point to the lower radial velocities RV Vs negative in order to conserve adequate RV colors in the graphs Half sector angle this is the half of the sector angle along the position angle PA Graph parameters a Frame Symbols Digits Legend amp add Jv Bele FEA oinez open square filled square Vmin Vmax defines the Y limits of the graph Rmin Rmax defines the X limits of the graph in pixels if the X scale is in pixels in arcsec if the X scale is in arcsec X scale pixels or arcsec In case of arcsec the scale arcsec per pixel is required Graph size
91. driver for contro display is a VCF file indicating the monitor driver for the control monitor plugged on the Matrox board The following VCF files are normally present in the ADWIPCS EXE directory VM101_60 VCF 640x480 60 Hz not recommended VM101_72 VCEF 640x480 72 Hz not recommended VM103_60 VCF 800x600 60 Hz OK for Thomson or DALSA 512 file C ADHOCw HELP adwi_f htm 3 of 5 15 02 02 09 34 01 ADwIPCS configuration files VM103_72 VCF 800x600 72 Hz VM105_60 VCF 1024x768 60 Hz OK for Thomson DALSA 512 or 1024 VM105_72 VCF 1024x768 72 Hz VM107_60 VCF 1280x1024 60 Hz VM107_72 VCF 1280x1024 72 Hz VM11C_60 VCF 1600x1200 60 Hz VM11C_72 VCF 1600x1200 72 Ha WARNING THE ADWIPCS PROGRAM NEEDS TO HAVE A CONTROL MONITOR ACCEPTING IMAGES OF THE SAME SIZE THAT THE DETECTOR If not there is a Matrox MdigGrab error Thomson needs at minimum 256 vertical lines DALSA AsGa 512x512 needs at minimum 512 vertical lines DALSA AsGa 1024x1024 needs at minimum 1024 vertical lines HOW TO CHECK THE CAPABILITIES OF THE CONTROL MONITOR load a DEF file with the VCF chosen driver press the Check Matrox PF key ask for Single message on screen if the OK message is visible this means that the monitor accepts this driver i e the dimensions and scanning rate which are specified in the VCF driver NOTE the first lines of the DCF or VCF drivers explicit the characteristics of the driver Comment
92. file C ADHOCw HELP adwt1_a2 htm 2 of 3 15 02 02 09 34 21 2 93 65 0 65 165 2 65 3 65 4 65 5 65 51165 6 65 17 6 38 6 59 6 80 6 01 6 22 6 43 6 64 6 85 6 05 6 26 6 47 6 68 6 89 6 10 6 31 6 52 6 73 6 646 656 665 675 684 694 704 TUS 723 732 742 751 761 770 780 790 799 809 818 828 837 847 856 866 876 885 895 76 77 77 AE 77 Th 78 78 78 578 579 59 579 D ADS 579 580 580 580 580 580 581 581 581 581 581 582 582 3 78 32 87 42 97 54 08 63 18 75 30 85 39 94 51 06 61 15 70 27 82 Sif 92 49 03 58 13 3 94 25 30 56 ZT 98 19 40 61 82 03 24 45 65 86 07 28 49 70 91 12 33 54 75 99 16 37 ADwT1 Channels tabulation Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located on the adhocw help adhocw htm file This file is adwt1_a2 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_a2 htm 3 of 3 15 02 02 09 34 21 ADwT1 precessions and heliocentric corre
93. for the Matrox board This value must be tuned and set with the Test Matrox function TV white level is needed for the Matrox board This value must be tuned and set with the Test Matrox function CS100 interface is the manner to drive the Queensgate Controller It could be parallel or serial For ESO it is O parallel interface For OHP it is 2 CON2 serial interface If there is no CS100 the user can put here a dummy value and then indicate on the menu that the scanning is not performed Shutter system can be O no shutter 1 OHP 2 Chili 3 AsGa or more depending of the further systems THT system can be O no shutter 1 OHP 2 Chili 3 AsGa or more depending of the further systems CCD X size is the physical horizontal CCD size to read It is 768 for Thomson and 512 or 1024 for DALSA AsGa depending if there is or not an hardware binning file C ADHOCw HELP adwi_f htm 2 of 5 15 02 02 09 34 01 ADwIPCS configuration files CCD Y size is the physical vertical CCD size to read It is 288 for Thomson and 512 or 1024 for DALSA AsGa depending if there is or not an hardware binning Stored image X size is the size of the recorded photons X addresses For DALSA AsGa it is usually the same value that CCD X size there is no interest to decrease the size of the photon addresses witch can be binned later by software For Thomson this value is 256 Stored image Y size is the size
94. image whithout any dialog Beinitialize colors a Load palette x Quit without saving bi Save a palette The palette will be stored and loaded for every ADw2D or ADw3D execution until it will be changed In addition it is possible to record a copy and reload it in a specific ADJ file To change a color simply click on the colored square corresponding to this color With basic colors and also personalized colors almost all the visible palette of colors 65536 are selectable file C ADHOCw HELP adw_uspa htm 2 of 3 15 02 02 09 33 50 ADw2D and ADw3D user palette Couleurs Couleurs de base Teinte QE Rouge ER Satur EJ Vert free Couleur rie Lum Fra Bleu i 70 Ajouter aux couleurs personnalis es Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_uspa htm Return to main ADHOCw menu file C ADHOCw HELP adw_uspa htm 3 of 3 15 02 02 09 33 50 ADw2D mixing different displays of images ADwT1 Return to main ADHOCw help Return to main ADw2D help Composition with several im
95. in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_f2 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_f2 htm 8 of 8 15 02 02 09 34 33 ADwT1 menu PYTHEAS ADwT1 Return to main ADHOCw help Return to main ADwT1 help Procedures to reduce TIGER and PYTHEAS TIGER F01 F02 PYTHEAS F01 F02 G01 F01 TIGER spectra position extraction from continuum image F02 TIGER creation of the 3D wavelength cube G01 PYTHEAS creation of the 3D wavelength cube CONTINUUM AD TIG E R data reduction procedure TIGER_pos TXT a file C ADHOCw HELP adwt1_tp htm 1 of 3 15 02 02 09 34 33 ADwT1 menu PYTHEAS TIGER_pos TXT CALIB AD OBJECT AD PYTHEAS _coef ADH Ina newe TIGER directons PYTHEAS data reduction procedure Omer Ina newe PYTHEAS directons file C ADHOCw HELP adwt1_tp htm 2 of 3 15 02 02 09 34 33 ADwT1 menu PYTHEAS Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be direct
96. interferometer tests THT and shutter management IPCS acquisition Tuning the system before acquisition ADW3D display as slave program of ADwIPCS file C ADHOCw HELP adw_ipcs htm 1 of 2 15 02 02 09 33 58 ADwIPCS This program requests a minimum screen of 1280x1024 with 256 colors and 96 pixels per inch If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwipcs htm Return to main ADHOCw menu file C ADHOCw HELP adw_ipcs htm 2 of 2 15 02 02 09 33 58 ADwIPCS Parameters Return to main ADHOCw help Return to main ADwIPCS help IPCS acquisition parameters When ADw3D launched the following window appears ADwIPCS The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page LPH T
97. interlacing gt Jf OK 7 Help file C ADHOCw HELP adw3d_z htm 3 of 4 15 02 02 09 33 58 ADw3D acquisition modes Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_z htm Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_z htm 4 of 4 15 02 02 09 33 58 ADwIPCS ADwIPCS ADHOCw program to acquire photon counting observations launches also ADw3D Return to main ADHOCw help This program acquires IPCS observations Intensified Photon Counting System from a TV intensified camera counting the photons The TV signal enters directly on a MATROX Genesis card PCI in the computer itself Almost all the TV formats up to 2000x2000 and frequencies can be managed see Matrox technical information The input frame frequency samples the chop This system is presently used at Haute Provence Observatory OHP for the GHASP experiment and at ESO for the 3m60 CIGALE and 36cm survey of the Milky Way and of the Magellanic Clouds IPCS acquisition parameters DEF configuration files TV and
98. is no information on the possible internal errors of the matrox board for example when the flux is to high to center correctly It is not important because the software introduces the notion of efficiency which allows to control this The full MIL errors mode is not recommended because it slows the speed down but this mode can be useful to test the system So the normal MIL errors mode if highly recommended Base default instrument parameters This allows to quickly get the correct parameters for different sites New it is now possible in case of failure to inhibit the shutter or THT controls by pressing the Inhib corresponding button located at the right of the value There is also an Inhib close loop button The correct values must be reload from the GHASP or Chile defaults THT low level is the THT voltage which is automatically reached as first step when tuning the very high voltage Usually there is no risk for the tube at this voltage even in case of bright illumination Photons usually don t appear THT medium level is the THT voltage which is automatically reached as second step when tuning the very high voltage Usually there is a risk for the tube at this voltage for bright illumination but file C ADHOCw HELP adwi_a htm 3 of 7 15 02 02 09 34 00 ADwIPCS Parameters not for common observations Photons begin to be visible THT maximum is the physical maximum THT voltage The user must control the flux o
99. lambda 6562 78 Angstroems Object scanning lambda 6571 64 Angstroems Object mean radial velocity 0 00 km s Heliocentric correction 0 00 km s file C ADHOCw HELP adwt1_a2 htm 1 of 3 15 02 02 09 34 20 ADwT1 Channels tabulation Object lambda at mean RV Interfringe Interfringe One channel One channel Reference dephased channel 1 1 Channels gt wavelength Chnl LO I AO BWNH EH AINA HBWNE NNNNNNNDN YO UP NN D H Lo 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 654 Be BW WWW Ww Ss OO OO I I JO OO O O O1 O1 O1 e e 2 Channels Chnl LU I oO O1 amp NH I Oo OU amp amp N DH N N t H Lo 22 23 24 25 26 27 900 891 66 L 872 862 852 843 833 824 814 805 195 486 FO 767 T9 STAT 138s 728 119 109 700 690 681 671 616d 652 3 06 27 48 69 90 SLT 32 5 93 74 729 25 36 sou 78 99 20 41 62 83 04 229 45 66 87 08 29 50 3 HT 20 66 ri 56 99 44 89 35 80 23 68 T3 59 04 47 92 37 82 25 71 16 61 06 49 94 40 2 6548 6548 6549 6549 6549 6549 6549 6550 6550 6550 6550 6551 6551 6551 6551 6551 6552 6552 6552 6552 6552 6553 6553 6553 6553 6553 6554
100. mean of all channels 3 Value n n channel number in decreasing order number in channel number in decreasing order order only ifoper 3 0 only ifoper 3 0 oper E emiss emission or absorption 0 emission 1 absorption Note 1 chg_chnls and pc _ mono exclude themselves Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information file C ADHOCw HELP adwt1b13 htm 3 of 4 15 02 02 09 34 44 ADwT1 continuum substraction boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b13 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1b13 htm 4 of 4 15 02 02 09 34 44 ADwT1 correction of wrong lines columns channels ADwT1 Return to main ADHOCw help Return to main ADwT1 help B14 Correction of wrong lines columns or channels py ADw correct wrong data ADHOCw ferecran Giarang fares Columns af amp 20 WE Lerecan Gi BORG ES cofumnrs ar Chaarels af a Fife Input 20 or 3D file Choose file Output 2E
101. name is also possible Xnnnnnnncccckkkk ADA One single ADA file contains the successive photon addresses obtained during a basic channel acquisition The ADT file name is Xnnn ADT The dialog window appears as file C ADHOCw HELP adw3d_z htm 1 of 4 15 02 02 09 33 58 ADw3D acquisition modes ADHOCw Origin of the data cubes Code of the observation r Cycles to integrate Indicate here one of the input data files Choose file Start cycle M a End cycle 9999 J iS ADA files 2 bytes coordinate se a MV Seesaw mode for scanning usually checked ans ok the onal Re scanning alternatively channels 1 gt n and n gt 1 Dimx 256 Dimy 256 Nbchannels 24 H m Normally DimX 256 and DimY 256 Binning 1x1 C 2x2 C 4x4 C 8x8 C 16x16 X Cancel 7 Help IPCS 4 or 6 bytes coordinate this mode can also be used during photon counting observations or later to integrate back already done observation for other image formats than 256x256 In this case the user must indicate the format and the possible presence of the frame count for deep photon counting statistics The ADA and ADT file names have the same rules as the IPCS 256x256 case above See saw follows the acquisition sequence in see saw mode See saw scanning mode organizes the scanning in order to scan in increasing mode the odd cycles scans and in decreasing mode the even cycles If this box is not checked all th
102. of 6 15 02 02 09 34 42 ADwT1 spatial smoothing This optional file which can be stored by pressing the Save user values button retrieved by pressing the Load user value button or edited with a common text editor is an ASCII file lts structure is the following The number of values must be 289 17x17 Number of spaces is not important and 303 342 1 Spatial 385 43 476 519 556 58 588 58 556 Jog Ge Che I uae uae uu uu IL ui 476 43 385 342 303 342 H Il WwW ee re 392 CD CDi OD 1D O0 Cr 0 Cr C6 6 0 6 C5 Or 60 C 449 Ll Le Ce Ce Ce CI ig IL ui lL Lu Ld all what is on right can be suppressed Macro definition Example SMOOTHXY fin D A fout keyword D ADHOCwS_plus BLA DHOCws_plus BLAI smoothing user file and SOUS Call da3 SOUS bidon ad3 square 3 content file C ADHOCw HELP adwt1_b9 htm 4 of 6 15 02 02 09 34 42 options note ADwT1 spatial smoothing SMOOTHXY fin 2D or 3D input file name with en 7 path 2D or 3D output file name with fout whole path square nb of binned adjacent channels see Note 1 below gauss half maximum width in channels see Note 1 below lorentz half maximum width in channels see Note 1 below 4 gt detail other 0 gt smooth 5 gt edge enhance 1
103. of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htmfile This file is adwt1_h3 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h3 htm 3 of 3 15 02 02 09 34 58 ADwT1 tuning ADwT1 Return to main ADHOCw help Return to main ADwT1 help H04 Instrument tuning using image sequences ADw tuning the instrument ADH OCw Tuning the Instrument using sequence Gf exposures TARA ADA photon counting 2 bytes photon 2564256 ADA photon counting a bytes photon Other dimensions ADA photon counting 8 bytes photon Other dimensions frame counting 4D2 or DAZ integrated images FITS integrated images Input 20 file 01 PP DatalGodboutiealog ad2 Choose file Suppress Input 2D file 02 DiData Godboutcalt0 ad2 Choose file Suppress Input 20 file 03 paDataiGodbouticaltt ad2 Choose file Suppress Input 2D file 04 iWata Godbouticali2 ad2 Choose file Suppress Input 20 file 05 DibataiGodboutical3 ad2 Choose file Suppress Input 2D file 06 DADataiGodboutcat sada sts Choose file Suppress Input 20 file 07 baDataiGodbouticaltS ad2 Choose file _Suppress Input 2D file 08 DADataiGodbouticah ad2 Choose file _Suppress Input 2D file 09 DaDatalGodbouticaltT ad2 Choose file Suppress Input 2D file 10 DADataiGodboutcats ada Ss Choose file Suppress Input 2D file 11 PP DatalGodboutieagad 0s Choose fil
104. of the cubes Extraction comer x 512 Y 512 Z a7 xO fi Y fi 70 ji Spectral information Perot Fabry Interferometer Re ah eroir an ry Interference order p h162 at 6562 780 Angstroems i Spectrography Wavelengths in Angstroems Calibration Object Line 6598 953 Line 6562 780 Scan 6598 953 Scan 6571 640 Length of spectra or interfringe 5 64 Angstroems km s Wavelength of channel 4 6559 957 Angstroems Velocities in km s Other parameters Mean RY of the object 0 000 km s Image scale 1 000 arcsec pixel Heliocentric RY correction 0 000 km s af Save on ADP file 7 Help x Abort don t save Identification is a free ASCII text written by the user to recognize his observation Dimension of the cubes have no limitations Z is usually the lambda dimension which is often the number of channels Extraction corner is a user information which keeps track of a possible further extraction from a larger cube all positions are numbered from 1 file C ADHOCw HELP adwt1_a1 htm 2 of 4 15 02 02 09 34 19 ADwT1 Basic 3D parameters Spectral information allows 2 modes the Perot Fabry mode and the Spectrography mode In the Perot Fabry mode you give the interference order of the interferometer relative to a given wavelength which is completely disconnected from the line wavelengths or the scanning wavelengths You must also give the line and scanning wavelengths for both calibration and object When
105. only be done from a dephased cube So you will built such a temporary cube just to identify the not polluted areas compute a temporary lambda cube function C02 of the ADwT1 program OBJ3 AD3 PHAS PRB AD2 gt LMBD_TMP AD3 identify areas zones which are free from the object spectrum and create a ADZ file from the zone function of the ADw3D program display LMBD_TMP AD3 and define zones in the sum folder Note that the ADZ file is compatible with the zone file issued from the old ADHOC DOS function 48 You will create for example the file ZONES _OH ADZ 9 correct from the transparency and sky background variations get the photometric parameters for correcting the transparency and the sky background inside these zones from the not dephased cube but corrected from cosmics function C05 of the ADwT1 program OBJ3 AD3 PHAS PRB AD2 ZONES OH ADZ gt PHOTOM ADX The photometric parameters are always written as an ADX file correct the original not dephased cube but corrected from cosmics function B15 of the ADwT1 program OBJ3 AD3 PHOTOM ADX gt OBJ4 AD3 10 test the result file C ADHOCw HELP adw_proc htm 3 of 5 15 02 02 09 34 47 ADHOCv Typical reduction procedure passing a second time the analysis for photometric parameters function C05 of the ADwT1 program OBJ4 AD3 ZONES OH ADZ gt TEST ADX look to the ASCII PHOTOM ADX and TEST ADX files PHOTOM ADX will show
106. or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file file C ADHOCw HELP adwi_f htm 4 of 5 15 02 02 09 34 01 ADwIPCS configuration files This file is adwi_f htm Return to main ADHOCw menu Return to main ADWIPCS menu file C ADHOCw HELP adwi_f htm 5 of 5 15 02 02 09 34 01 ADwIPCS tests ADwIPCS Return to main ADHOCw help Return to main ADWIPCS help IPCS TV and interferometer tests The level determination is very important it changes even during one night and the user must check in permanence that the efficiency of the system is maximum This can be done by looking regularly to the second TV VGA monitor which displays the work of the MATROX board But the user can also check every thing before the observation file C ADHOCw HELP adwi_b htm 1 of 4 15 02 02 09 34 02 ADwIPCS tests i 7 ADHOCw Test Matrox Genesys Board and Imaging Library MIL ADHOCw Test Matrox Genesys Board and Imaging Library MIL Some of these test and demonstrations functions of the Matrox Genesys board require an additional screen display which must
107. present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_ass htm Return to main ADHOCw menu file C ADHOCw HELP adw_ass htm 6 of 6 15 02 02 09 35 05 ADHOCw is used in about 30 sites in the world ADHOCw runs in about 30 sites in the world file C ADHOCw HELP adwworld htm 15 02 02 09 35 06 ADHOCw software installation ADHOCw Return to main ADHOCw help Software installation This is the readme txt file for software installation The ADHOC software is available freely on the Web at the adress http www obs cnrs mrs fr adhoc adhoc html in a unique compressed ZIP file of 6 Mb The sucessive versions are numbered 98A 98B 99A 99B 99C 00A OOB depending of the year of release The zip file name refers to the version ADW_99A ZIP for instance The following files must be retrieved adw_99A zip executables and help readme txt this file history txt history of the modifications copy_scr zip screen copy utility 1 To install the software unzip ADw99A ZIP or further version with a WinZip like program http www winzip com Note
108. printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_y htm Return to main ADHOCw menu Return to main ADw2D menu file CI ADHOCW HELP adw2d_y htm 2 of 2 15 02 02 09 33 48 ADw2D main display screen ADw2D Return to main ADHOCw help Return to main ADw2D help Main 2D display screen After opening a 2D file or a context file you will get a windows of the following aspect The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page SR ADHOCw 2D display no ADC context TH src Bones mer hee eo Piz EA Fan leu 7 BHF Seir pistes iman rartext dar X item z DAME apse Whos wimage xj Darmar Image Main image Nar 131Go hit liar d tele thor ol ees Miisu 2eisrahers 7 ere ent O aega rev al pan Fig veal l Fiphozoriay sags macficaicr oh ae zila ERI Reiazcw f Whemedseoss s4 Le ELA Vey 27x12 TJ Smor ca TEU Wer UIE WILD Em me zwu Lous seule pa sits ene JaA hinkress fo a rihh Lamas J mele aa i fees 10 5 hilt raise recht dire ws 42 ALL mc Vina eli mee FT ane an fie Smrcathac pi a at 424 twl 32 Sem A Ezels cverep yAachos al Leta Page folders You can access to t
109. r V plot is drawn This appearance is similar to this D ADHOCw ADw2D kinematics i al alty adr all 4 quadrants E 2 RSC CROWNS bluered Me Ton Save graph as BMP z Siea asliii 30 00 e 133 00 121 00 2320 00 TA aol FiA oaint M file C ADHOCw HELP adw2d_k1 htm 9 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph SA salty paint M RE M A thickness pixels thickness of the band along the major axis 2D threshold isophotes threshold 2D step isophotes step Recommended values in order to help the user the program computed approximate values for threshold and step From these basic values which usually show something it is possible to improve the expected graph Nb maxi isophotes in order to improve the graph the user can limit the number of isophotes The lower isophotes will always be drawn The brighter ones will be absent Mass distribution Hass distribution This function is not yet implemented Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file
110. random values for A and B for TEST ADX the A and B values will be almost constant This confirms that the correction was good E Get the lambda cube 11 compute the lambda maps function C02 of the ADwT1 program OBJ4 AD3 PHAS_PRB AD2 gt LMBD AD3 E Suppress OH 12 suppress night sky OH pollution by using the function C04 of the ADwT1 program LMBD AD3 ZONES OH ADZ gt LMBD_OH AD3 Use the default parameters as first approach F Get the lambda cube and the monochromatic continuum radial velocities maps 13 compute monochromatic continuum radial velocities maps put the good heliocentric velocity correction function A03 of the ADwT1 program You can also use the old ADHOC DOS function 48 and enter the value with the function A01 of the ADwT1 program execute the function C03 of the ADwT1 program LMBD OH AD3 gt MONO_ORG AD2 CONT_ORG AD2 RV_ORG AD2 WIDTH_ORG AD2 Use the default parameters as first approach If you cleaned the cube from CCD photometrical variations along the exposure look to the efficiency of the method build monochromatic continuum and radial velocity maps from the not corrected cube with the function C03 of the ADwT1 program LMBD_TMP AD3 gt MONO_TMP AD2 CONT_TMP AD2 RV_TMP AD2 use ADW2D function of superposition to compare MONO_TMP AD2 with MONO_ORG AD2 CONT_TMP AD2 with CONT_ORG AD2 and RV_TMP AD2 with RV_ORG AD2 G Cook yourself your file
111. spectra of width 6 pixels 2 0 4 Nb spectra of width 7 pixels 0 0 0 All the spectra are normalized to a height of 5 pixels FINAL Nb spectra of width 1 pixels 0 0 0 FINAL Nb spectra of width 2 pixels 0 0 0 FINAL Nb spectra of width 3 pixels 0 0 0 FINAL Nb spectra of width 4 pixels 0 0 0 FINAL Nb spectra of width 5 pixels 547 100 0 FINAL Nb spectra of width 6 pixels 0 0 0 FINAL Nb spectra of width 7 pixels 0 0 0 Writing control images Drawing positions Storing positions ADVT1 TIGER 1 0009 09 Lower 16 50 49 F01 TIGER_POS Info Correct end Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_f1 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_f1 htm 8 of 8 15 02 02 09 34 34 ADwT1 PYTHEAS 1 ADwT1 Return to main ADHOCw help Return to main ADwT1 help G01 PYTHEAS creation of the 3D wavelength cube How to reduce PYTHEAS Function G01 This function is the third step for PYTHEAS data reductions after F01
112. tabz_ref 4 912 372070 0173 01 Lower 17 58 19 k tabz ref 5 912 347839 0173 01 Lower 17 58 19 k tabz ref 6 912 459045 0173 01 Lower 17 58 19 k tabz_ref 7 912 474243 0173 01 Lower 17 58 19 k tabz_ref 8 912 343872 0173 01 Lower 17 58 19 k tabz_ref 9 912 323120 0173 01 Lower 17 58 19 k tabz_ref 10 912 398621 0173 01 Lower 17 58 19 k tabz ref 11 912 370605 0173 01 Lower 17 58 19 k tabz_ref 12 912 381348 0173 01 Lower 17 58 19 k tabz ref 13 912 407166 0173 01 Lower 17 58 19 k tabz_ref 14 912 417664 0173 01 Lower 17 58 19 k tabz ref 15 912 440063 0173 01 Lower 17 58 19 k tabz_ref 16 912 358032 0173 01 Lower 17 58 19 k tabz_ref 17 912 301514 0173 01 Lower 17 58 19 k tabz_ref 18 912 318054 0173 01 Lower 17 58 19 k tabz ref 19 912 425293 0173 01 Lower 17 58 19 k tabz_ref 20 912 370117 0173 01 Lower 17 58 19 k tabz ref 21 912 395813 file C ADHOCw HELP adwt1c11 htm 5 of 8 15 02 02 09 34 53 ADwT1 rough photometry 0173 01 Lower 17 58 19 k tabz ref 22 912 445496 0173 01 Lower 17 58 19 k tabz ref 23 912 395569 0173 O01 Lower 17 58 19 k tabz_ref 24 912 436584 0173 01 Lower 17 58 19 k tabz_ref 25 912 365112 0173 01 Lower 17 58 19 k tabz_ref 26 912 429810 0173 O01 Lower 17 58 19 k tabz_ref 27 912 474121 0173 O01 Lower 17 58 19 k tabz_ref 28 912 772522
113. the phase map get the scanning wavelength information from the observation and insert these values in the parameters function A01 of the ADwT1 program get the approximate center of the rings of the calibration ADw3D program compute the phase map function C01 of the ADwT1 program CAL AD3 gt PHAS_PRB AD2 and give here the wavelength or channel 1 the values of the approximate center of the rings if CCD X Y must be forced to 1 If IPCS it must not be forced check the image RV_cal AD2 with the ADw2D program the mean value of the background must be around 0 km s If the cross section shows a variation from the center to the outer parts it is normal and comes from the fact that the interfringe is different for the object and for the calibration 4 in the case of 2 phase maps one before observations and one after simply mix both parabolic phase maps with the function B06 of the ADwT1 program Parabolic phase can easily be averaged by this simple function You can enter different weights for every phase map The resulting parabolic phase map will be used for the next steps instead of one of the parabolic phase maps C Get a clean original object cube 5 for CCDs observations in any case correct the pure not dephased original object file C ADHOCw HELP adw_proc htm 2 of 5 15 02 02 09 34 47 ADHOCv Typical reduction procedure cube from cosmic rays function B12 of the ADwT1 program
114. the program Help Session log book see the ADL log file for the full history of all the sessions F Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions E01 Integration time normalization and remanence cleaning of ADA files file C ADHOCw HELP adwt1_e htm 1 of 2 15 02 02 09 34 55 ADwT1 menu IPCS Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_e htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_e htm 2 of 2 15 02 02 09 34 55 ADwT1 menu TIGER ADwT1 Return to main ADHOCw help Return to main ADWT1 help Tiger functions F How to reduce TIGER AD aDwT1 sh152 j 10 x Hide task manager window i Version l Bring task manager to front AD H OCw ADwT1 2001E JBx Obs Marseille 1280 s 1024 96 ppi General 2D 3D operations Cigale Profiles IPCS Tiger Pytheas misce
115. the spectral lamp and the calibration scanning wavelength can be found in the logbook of the observation the object line is at the zero velocity and the object scanning wavelength can be found in the logbook of the observation the object radial velocity is used here in order to compute later the radial velocities at the correct order If this value is false a modulo error of the interfringe can exist the heliocentric radial velocity is an additional correction which is obtained from the A03 function The wavelength of channel 1 will be the reference of channel 1 for dephased cubes It can be what you wish but two values are predefined the calibration wavelength in case of doubt the object channel 1 will be in phase with the calibration rings or better the mid spectrum in this case the object line will be put in the center of the dephased spectrum which is more comfortable for the 3D displays file C ADHOCw HELP adwt1_c1 htm 2 of 6 15 02 02 09 34 17 ADwT1 phase computation The center of the rings is important because it is necessary to modelize the phase during its computation You can get these coordinated by using the ADw3D program and displaying the calibration cube These coordinates are numbered from 1 and can be located outside of the images values lt 1 or gt size XY The center of the rings can easily be obtained from the visualization of the calibration cube with the ADw3D program The X Y pixel rat
116. the user press the button Update values the interfringe values in Angstroems and in km s are automatically computed The wavelength of channel 1 is the reference wavelength for the de phased cubes This last parameter can be changed until the phase map computation In the Spectrography mode the only useful parameters which must be given by the user are the length of the spectrum in Angstroems and the wavelength of the first spectral element When the user press on the button Update values the length of the spectrum in km s is computed Velocities are necessary to compute the correct radial velocities maps The mean velocity of the objects allows the program to compute at every pixel the best interference order avoids modulo The heliocentric radial velocity correction is relative to the date of he observation and the position of the object This last value can be computed in the menu A of the program Other parameters are additional information The image scale is useful for complex functions as dynamics It can be changed at any time and many functions don t use this value which can be let to 1 at the beginning The modifications must be then saved onto the ADP parameter file lf the ADP parameter file name changes the history file ADL file name also changes the command numbering will begin to 0 and the ADL file will be created again 3 ADw warning ADHOCw warning ou requested to save the parameters ina ne
117. threshold is in monochromatic map intensity units Displayed profile in the top zoom box can be interferograms or wavelength maps Wavelength maps are usually the best Computation parameters The user must give the basic parameters Perot Fabry parameters Phase reference wavelength identical to the ADwT1 C01 parameters which built the parabolic phase map loaded in the phase folder Scanning wavelength relative to interferograms Zero velocity wavelength relative to the observed object Mean radial velocity in order to shift radial velocities in the correct range modulo of the interference order RV correction Ex heliocentric can be computed from the A03 ADwT1 function Profile type emission or absorption computation Spatial smoothing in order to increase the S N on profiles and measure values in faint areas Can be none up to 25x25 pixels OH suppression if a ADZ zone file is given the OH can be suppressed from the individual profiles before computation The ADZ file can be created from the Sum folder In this case the OH profile in the zones appears on the display Substracted OH profile Typical velocity field obtained in real time during observations ADHOC 3D main display panel 3D file lambzlisg5 ad3 0112 40 Cube dimensions x 256 ly 256 lz 2a Mouse profile area fi 1 pix X Printer setup Print screen M Retresh at every channel Save 3D data fi 2 Waiting gap sec 7
118. to have OH night sky lines but the method works also without any sky line because it can work on the continuum itself We assume that every CCD channel must be corrected from photometry in the following way real_value a measured_value B In a first step we will compute the inverse function measured_value a real_value b for every channel For this the sum of the rephased profile is computed for every pixel the profile is rephased from the parabolic phase and summed in a single array This summed profile is given in the output log file as k tabs ref This rephased profile is supposed to be the real_value because it is obtained from all the observed channels during the whole observation exposure time Then every channel is analyzed For every pixel the value of the rephased channel is computed This is the measured value By this way we can draw a graph in which the X is the real_value of the integrated rephased channel all aver the exposure normalized with the number of pixels and Y is the measured value of the rephased channel for every pixel The square mean algorithm gives the a and b values of the measured value a real_value b equation There are k equations k being the number of channels and therefore k values for a and b In a second step a k and b k values are converted to a k and B k values in order to convert all the original not rephased or original not rephased corrected from cosmic rays and or
119. to minimize the least square deviation of the rotational velocity within the successive crown sectors All the cases are computed amp Dw2D minimizing parameters 10 x ADw2D optimizing crowns parameters for rotational velocities to 1100 M Symetrize radii Numer of crowns 10 V Let vary Xe from 116 to IV Let vary Ye from 126 to Let vary MA fr now fixed 155 00 IV Let vary Ys r from 900 Let vary incli fr now fixed 30 00 Nb of iterations 525 Return to image 7 Help kisa Xc 120 00 Yc 130 00_MA 55 0 Vs sate 0 ra areal mean weic 2522 120 00 E O0 55 00 120 00 130 00 55 00 120 00 130 00 55 00 120 00 130 00 55 00 120 00 130 00 55 00 file C ADHOCw HELP adw2d_k2 htm 10 of 12 15 02 02 09 34 27 1000 00 1000 00 1000 00 1000 00 1000 00 124 134 30 00 30 00 30 00 30 00 30 00 3 1 3 5 41 5 2 7 2 step 2 step 2 step fio E 3 54 1 71 3 55 7 35 9 Xc Ye center of the curve MA position of the major axis in degrees direct sense 0 at top Vs systemic velocity in km s Incli inclination in degrees with respect to the sky plane Save results into TXT file Crowns detail RES TST Previous Nest i ae Get detail for crowm number gt 1 am Displayed crown 1 Crown parameters 116 0 Minimized xc 120 0 123 0 ADw2D kinematical functions user made crowns Minimized Ye 130 0 Minimized PA
120. to replace some characters by some in order to indicate where the number of the channel will be introduced You can give a first channel number default 1 which will be the first number The number of must be sufficient to code the last channel first nb_chan 1 For example Reference channel YA120212 FIT First channel 13 Number of channels 24 Mask YA1202 In this case the slice files will be YA120213 FIT to YA120236 FIT 3 to validate the file names and their channel order At this step a 2D table appears You can modify as you wish the names of the files inside the table You can change individually the file names You can change the channel order For CFHT observations which are interleaved i e the scanning order is not simply increasing you can get the true information of the interleave by using the Automatic CFHT ordering checkbox In this case Fits headers are read in order to find the CURCHAN value which indicates this information At the end when you press the key continue for execution the existence of the slices are checked if slices are as input Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML file C ADHOCw HELP adwft_a2 htm 3 of 4 15 02 02 09 34 07 ADwET slices help can be directly accessible to your favorite HTML browser Netscape IExp
121. to the left of the image 180 if the PA points to the bottom of the image and 270 if the PA points to the right of the image It is recommended to point to the lower radial velocities RV Vs negative in order to conserve adequate RV colors in the graphs Half sector angle this is the half of the sector angle along the position angle PA Quadrants quadrants are numbered 1 2 3 and 4 as graphically shown in the window Possible modes are full image 4 quadrants only quadrant 2 quadrant 3 in position 2 r and V inversed quadrant 4 in position 2 V inversed superposition of quadrants 1 and 3 in position 2 superposition of quadrants 2 and 4 in position 2 file C ADHOCw HELP adw2d_k htm 4 of 6 15 02 02 09 34 24 ADw2D kinematical functions case of 4 quadrants case of quadrant 3 in position 2 Points crowns there are 3 possibilities points are drawn in the same colors than the points of the 2D image as graphs above real colors points are drawn with only 2 colors blue and red corresponding to the different quadrants points are not drawn but crowns are computed The mean value and sigma are computed inside crowns of p The parameter thickness of the crown is free Rmin Rmax defines the X limits of the graph Vmin Vmax defines the Y limits of the graph Redraw graph redraws the graph when the values and or parameters are manually changed If file C ADHOCw HELP adwa2d_k htm
122. ue cme ater ui Ars Ny Choose Cepate D race F Paie nus evi ade den FAs soos d hy es Xa vk Cdkn force rofeldesine SRE om Came Dias HY te cn piis Views isien mede Jasedcd The right side of the window changed the mode for the Action of the left button of the mouse is now Integration of profile This means that the user can simply press on the left button of the mouse to select one profile which is immediately displayed on the right part of the window Pressing again will add profiles Pressing again on a previously selected profile will substract it file C ADHOCw HELP adw2d_e htm 3 of 8 15 02 02 09 33 54 ADw2D 3D profiles Integrated profile This profile is exclusively from 3D file 1 Profile in large window Nb cells 1 Nb pixels 1 Clear selection jirec a Barycenter I Absorption itetnge 411321 km s P 21 Press on the right mouse button to chop Current RY Chopped AY 320 2 km s Copy to 2D image 1 Undo 2D successive modifications Modify replace and store profile Cnl1 6520 00 ObiectO 6562 78 RVO 0 0 km s i 90 104 Cor 0 00 km s Draw RY tics on profile Measuring the profiles Moving the mouse in the profile graph allows to get the channel position the wavelength the radial velocity and the intensity of the pointed channel The measure can be direct the exact position of the mouse is taken
123. 00 x Append and save Overwrite and save Save medited o uit When you run the Store macro the status existing or not of the input output data files is not checked they could be created by a previous macro which is not yet executed To execute an existing batch you must press the Exec a batch file button in the window displayed below In this case the task manager will allocate the task 16 for the batch This means that only one batch can run at the same time in an ADHOCw session But several ADHOCw session can run simultaneously in different directories file C ADHOCw HELP adwt1_ba htm 2 of 6 15 02 02 09 34 07 ADwT1 batchs ADwT1 Pytheas 10 x Hide task manager window Version Bring task manager to front AD H OCw ADwT1 2001E JBx Obs Marseille l 1280 x 1024 96 ppi General 2D 3D operations Cigale Profiles IPCs Tiger Pytheas Miscell Compute monochromatic continuum radial velocities line widths 2D maps EA Edit a batch file 4 Substract OH and or continuum from given areas a Get photometric parameters from OH lines case of CCD gt ADX file ix Exec a batch file Get seeing analysis channel channel case of CCD gt ADS file Merging of several ADS seeing parameters files Photometric correction channel channel from seeing ADS file EA Show logbook Compute the calibration Finesse Build custom made lambda cubes fat Display control Get photometric paramet
124. 000 200000 Frecessions and abject VISENE 2 NGC 2601 le 25 12 00 e7 s7 loco 1950 00 3 Nac 5227 na 32 4800 1 ao looo 1950 00 bomputetor selected object select first object in the list Load object array from a file Click in the array to seclect an object Double click in the array to compute Save object array into a file This program allows to compute precessions and gives indication on the visibility of the object in a given site The user can build a list of objects This list is kept for the next execution of the program It is very easy to add an object to the list file C ADHOCw HELP adwt1_h6 htm 1 of 3 15 02 02 09 35 00 ADwT1 Precessions a0 ADw new object for precession OP x ADHOCw New object far precession Name Alpha Delta Epoch NGC 7764 23 48 i v4 lt x E jo 30 2000 h m deg a Add this object to the list x Quit without adding object Then the user has only to click on the given object in the list A new window opens the user must choose the site the date and the graph width 16 or 24 hours Pressing Execute shows the visibility graph with the air mass values Moving the mouse inside the graph indicates more accurately the air mass 8 ADw Object visibility ADHOCW Graph far ae ee on Name Epoch Selected object N GC 7764 23h if 400s F did ne a 000 2000 00 Longitude Latitude Print this window C
125. 000 x12 6610 0000 stepz 0 5000 lens 27 62800 n 0 fout D Pytheas SH152 cube sh152 brut ad3 fadp D Pytheas SH152 cube sh152 brut adp fpytheas D Pytheas SH152 PYTHEAS_coefficients ADH fverif2 D Pytheas SH152 cube verif_calib AD3 keyword content options TIGER_CUBE fo fcalib calibration 2D input file name with whole path fpos input TXT position file name with whole path from F01 ss fwi internal wavelength input file name with whole path ss file C ADHOCw HELP adwt1_f2 htm 5 of 8 15 02 02 09 34 33 ADwT1 TIGER 2 fverif verification 2D output file name with whole path fin input 2D observation file with whole path threshold calibration lines threshold height pixels to add to the central line for calibrations to add to the central line for calibrations mode alee eke wavelengths a a _ degree dispersion dispersion polynomial degree degree a x2 spectrum extension to the right sigma sigma elimination on positions wiref reference reference objectline line me ref precem o o ooo origin no rs space D XY sampling D XY sampling l T xl1 starting wavelength Angstroems fo xI2 ending wavelength Angstroems ss stepz wavelength step Angstroems ss lens L distance between lenses fo n number of the most intense calibration line 0 notest fout output 3D file in a different directory ss
126. 000 y1 101 000000 x2 200 000000 y2 201 000000 0019 01 Lower 22 13 11 Zone 2 x1 50 000000 y1 10 000000 x2 100 000000 y2 98 000000 0019 01 Lower 22 13 11 Zone 3 x1 1 000000 y1 2 000000 x2 8 000000 y2 9 100000 Multi pass substractions This mode is left here in order to be compatible with the previous ADHOC DOS software In some cases it is the way to control in the very detail the procedure and to minimize noise For CCD the photon noise is not so essential and the night sky lines substraction can be done in 1 pass with a file C ADHOCw HELP adwt1_c4 htm 5 of 6 15 02 02 09 34 15 ADwT 1 OH and or continuum substraction substraction factor of 1 For photon counting nevertheless the photon noise is important and the user can compute the substraction in several passes 3 for instance first the 1st substraction factor is subtracted then the second then the third It is strongly recommended to fix the last factor to 1 in order to have no residual The choice of the substraction factor at every pass can be computed from the photon noise In principle it is impossible to substract more than 1 noise signall i e 1 sqrt signal signal 1 1 sqrt signal where signal is the mean height of the OH line to substract This value of the substraction factor P 1 1 sqrt signal is maximal and must not be larger If not you will substract noise and obtain negative flux values But it is possible to redo this and substract
127. 00537 879370 447687 560732 513467 678005 191716 576296 395879 ADwT1 mixing ADS seeing files seeing 1 595770 pixels 0210 01 Lower 09 23 20 Channel 27 dx 0 950780 dy 0 596855 seeing 1 595770 pixels 0210 01 Lower 09 23 20 Saving control curves into BMP file 0210 01 Lower 09 23 21 Control graphic is buffered and can be displayed by pressing on the Display control button Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c7 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_c7 htm 5 of 5 15 02 02 09 34 50 ADwT1 ADwT1 Return to main ADHOCw help Return to main ADwT1 help C08 Seeing correction 8 ADw seeing correction OF x AD HOCw Seeing correction i Maximum seeing correction Waiting for input ADS file name Input not dephased 30 file Maximum seeing allowed in pixels Scroll to get information of the seeing values Input ADS seeing file Choose file Input 2D parabolic phase Choose file E ADH
128. 01 10 505 channels 0182 16 Batch Lower 18 16 28 G01 10 828 channels 0182 16 Batch Lower 18 16 28 G01 11 153 channels 0182 16 Batch Lower 18 16 28 G01 11 476 channels 0182 16 Batch Lower 18 16 28 G01 11 800 channels 0182 16 Batch Lower 18 16 28 G01 12 124 channels 0182 16 Batch Lower 18 16 28 G01 12 123 channels 0182 16 Batch Lower 18 16 28 G01 order found is 601 at 6562 780 0182 16 Batch Lower 18 16 28 G01 be used in computations 0182 16 Batch Lower 18 16 28 G01 output file 0182 16 Batch Lower 18 16 28 G01 individual lens spectra 0182 16 Batch Lower 18 16 28 G01 temporarily file 0182 16 Batch Lower 18 16 40 G01 547 0182 16 Batch Lower 18 16 43 G01 547 0182 16 Batch Lower 18 16 45 G01 PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info file C ADHOCw HELP adwt1_g1 htm 10 of 14 15 02 02 09 34 36 order 627 order 628 order 629 order 630 order 631 order 632 order 633 order 634 order 635 order 636 order 637 order 638 order 639 Result best interference This in
129. 0181 01 Lower 2 08 10 Analyzing channel 3 0181 01 Lower 2 08 11 a 0 921287 b 3 199606 0181 01 Lower 08 Analyzing channel 4 0181 01 Lower 08 a 0 773271 b 8 099334 0181 01 Lower 08 Analyzing channel 5 0181 01 Lower 2 08 12 a 0 889761 b 8 555343 0181 01 Lower 2 08 12 Analyzing channel 6 0181 01 Lower 2 08 12 a 0 824892 b 2 202654 0181 01 Lower 2 08 12 Analyzing channel 7 0181 01 Lower 2 08 13 a 1 012390 b 9 263886 0181 01 Lower 2 08 13 Analyzing channel 8 0181 01 Lower 2 08 14 a 0 855564 b 6 438394 0181 01 Lower 2 08 14 Analyzing channel 9 0181 01 Lower 2 08 14 a 0 832540 b 2 267165 0181 01 Lower 2 08 14 Analyzing channel 10 0181 01 Lower 2 08 15 a 0 812519 b 5 774867 0181 01 Lower 2 08 15 Analyzing channel 1 0181 01 Lower 2 08 15 a 0 905670 b 7 281686 0181 01 Lower 2 08 15 Analyzing channel 12 0181 01 Lower 2 08 16 a 0 975033 b 5 281760 0181 01 Lower 2 08 16 Analyzing channel 13 0181 01 Lower 2 08 16 a 0 888480 b 14 087481 0181 01 Lower 2 08 16 Analyzing channel 14 0181 01 Lower 2 08 17 a 0 992038 b 0 119689 0181 01 Lower 2 08 17 Analyzing channel 15 0181 01 Lower 2 08 18 a 0 885125 b 1 139048 0181 01 Lower 2 08 18 Analyzing channel 16 0181 01 Lower 2 08 18 a 0 882421 b 2 346781 0181 01 Lower 2 08 18 Analyzing channel 17 0181 01 Lower 2 08 19 a 0 852420 b 8 597904 0181 01 Lower 2 08 19 Ana
130. 05 54056 6520 100 404 75952 6520 200 405 40033 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_zp htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adwe2d_zp htm 6 of 7 15 02 02 09 33 56 ADw2D zoom on profiles file CIADHOCw HELP adw2d_zp htm 7 of 7 15 02 02 09 33 56 ADw3D 11 zones ADw3D Return to main ADHOCw help Return to main ADw3D help Defining profile zones in the 2D image This mode corresponds to the Sum folder The user can define up to 11 zones and display the integrated profiles in these zones The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page file C ADHOCw HELP adw3d_c htm 1 of 3 15 02 02 09 33 57 ADw3D 11 zones CE ADIIOU JU display men panci Cris E F t E L Ho woe ES HE DES LEE pes Heal time stim of the Imerterviirants Fat eet aa Le Isys wuns
131. 09 Lower 16 50 39 F01 TIGER_POS Info 0009 09 Lower 16 50 43 F01 TIGER_POS Info 0009 09 Lower 16 50 43 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 46 F01 TIGER_POS Info 0009 09 Lower 16 50 49 F01 TIGER_POS Info file C ADHOCw HELP adwt1_f1 htm 7 of 8 15 02 02 09 34 34 Reserving arrays Nb of roughly extracted spectra 2234 Nb of eliminated spectra too small 1687 Nb of remaining extracted spectra 547 Nb of remaining final spectra 547 Nb spectra of width 1 pixels 0 0 0 Nb spectra of width 2 pixels 28 5 1 Nb spectra of width 3 pixels 203 37 1 Nb spectra of width 4 pixels 273 49 9 Nb spectra of width 5 pixels 41 7 5 Nb
132. 1 23693 11 7664 channel 27 A and B for Y AX B file C ADHOCw HELP adwt1c11 htm 3 of 8 15 02 02 09 34 53 ADwT1 rough photometry From this C11 program B is always equal to 0 For the computation it is possible to use a reference photometric 2D file which is supposed for example to give an idea of the flat field through the filter instrument detector If this file is absent the reference values are considered to be 1 If the reference 2D file has null values they are not taken in account the reference sum of the profile is not incremented The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DAS This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example ROUGH_PHOTOM fin D Data IKI neb2_cos ad3 fzones D Data IKI zones2 adz mode_ref 0 fphotom D Data IKI truc adx fbmp D Data IKI truc bmp bkgd 0 keyword content options ROUGH_PHOTOM PHOTOM fne se input not dephased file name with whole path fzones ADZ input file containing selected areas fphotom ADX output file to store photometric coefficients mode_ref mode of 2D reference file 0 no file 1 file indicated in fref fref 2D photometric
133. 10 31 05 Chnl 24 New A Old B A 1 20471 1 426190 0272 01 Lower 10 31 05 Chnl 25 New A Old B A 1 10585 9 212370 0272 O01 Lower 10 31 05 Chnl 26 New A Old B A 1 28748 10 667800 0272 O01 Lower 10 31 05 Chnl 27 New A Old B A 1 23693 11 766400 file C ADHOCw HELP adwt1b15 htm 3 of 4 15 02 02 09 34 45 ADwT1 Photometric corrrection Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b15 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1b15 htm 4 of 4 15 02 02 09 34 45 ADwT1 photometry from OH ADwT1 Return to main ADHOCw help Return to main ADwT1 help C05 Get photometric parameters from OH lines CCD 14 ADw OH photometry ADHOCw Get photanmewe parameters fam OFF tres CCL Input orginal not dephased 3D file Choose file Input 20 parabolic phase map tile Choose file EADH OCwS plus BLAISOUSIESSATP has prh 4D2 Input ADZ ASCII zones Input file Choose file Output ates ASCI photometric parameters file Choo
134. 15 02 02 09 34 19 ADwT1 menu GENERAL A02 function Tabulated wavelength and velocity values per channel A03 function Computation of the heliocentric radial velocity correction Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_a htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_a htm 2 of 2 15 02 02 09 34 19 ADwT1 Basic 3D parameters ADwT1 Return to main ADHOCw help Return to main ADwT1 menu A01 General parameters of the cubes This function can be called at any moment The user must know nevertheless that some changes can affect the data reduction and lead to some confusion changing for example the interference order after the computation of the phase map gives obviously wrong results file C ADHOCw HELP adwt1_a1 htm 1 of 4 15 02 02 09 34 19 ADwT 1 Basic 3D parameters ADw parameters ADHOCw Basie aD parameters Identification File parameter nanO 4A0HOCws_pluz BLAISOUS Blaizous adp Object identification Dummy object Dimensions
135. 19 582 479 654 483 25 461 520 1 479 761 483 No measure 521 65 484 132 488 24 411 file C ADHOCw HELP adwt1_g1 htm 4 of 14 15 02 02 09 34 36 ADwT1 PYTHEAS 1 Output 2D verification file zero wavelength calibration interference order this file records the channel number of the first calibration line corresponding to the nearest micro lens Variation in these values indicates a bad tuning of the interferometer This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example PYTHEAS_CUBE fcalib D Pytheas SH152 P039 ad3 fin D Pytheas SH152 P038_no_cosmics ad3 p_pf 609 Imbd_p 6562 780 Imbd_scanobj 6630 000 mode_order 0 integ 1 x11 6520 0000 x12 6610 0000 stepz 0 1000 wlref 6562 780 fout D Pytheas SH152 pytheas sh152_pytheas ad3 fadp D Pytheas SH152 pytheas sh152_pytheas adp fpytheas D Pytheas SH152 PYTHEAS_coefficients ADH fverif D Pytheas SH152 pytheas PYTHEAS_zero_wl AD2 fverif2 D Pytheas SH152 pytheas PYTHEAS_zero_wl TXT keyword content options PYTHEAS CUBE fcalib calibration 3D input file name with whole path fin input 3D observation file with whole path pps approximatedorder Imbd p reference wavelength forthe order Imbd_scanobj scanning wavelength for object and
136. 1_a1 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_a1 htm 4 of 4 15 02 02 09 34 19 ADwT1 ADP parameter files ADwT1 Return to main ADHOCw help Return to main ADwT1 help ADP parameter files An ADP parameters file is absolutely necessary for the data processing This file has a similar function with the param cig files in the old ADHOC DOS software This ADP parameters file has a copy which is an ADQ suffix file If the ADP file is corrupted the ADQ file replace it automatically This avoids to loose the parameters file in case of disk or computer program The parameters of the ADP file can be changed by the user with the ADHOCw function A01 The ADP parameter files contain the following informations file C ADHOCw HELP adwt1_ad htm 1 of 5 15 02 02 09 34 20 ADwT1 ADP parameter files I ADw parameters ADHOCw Basie aD parameters dentification File parameter narm Object identification Dummy object traction corner imensions of the cubes x 256 256 C Spectrography avelengths in Angstroems alibration Object Line 6598 953 Line 6562 780 Scan 6598 953 Scan 6562 780 Length of spectra or interfringe 6 276 Angstroems 377 938 km s Wavelength of channel 4 6562 780 Angstroems her parameters Image scale 1 000 arcsec pixel Velocities in km s Mean RY of the object 0 000 km s Heliocentric R
137. 2 fout Jbx_portable D ADHOCWs_plus BLAISOUS bidonl ad2 oper 3 fsuper Jbx_portable D ADHOCWs_plus BLAISOUS Star txt subst 3 1 keyword content GEOMETRY fin 2D or 3D input file name with whole path fout 2D or 3D output file name with whole path operation type oper fsuper ASCII pixel reference file up to 100 lines shiftX pixels to shift in X positive or negative shiftY pixels to shift in Y positive or negative ishiftZ channels to shift positive or negative to shift channels to shift positive or negative or negative C SE EE ee rotation angle in the direct sense and in degrees positive or negative Kes me X X rotation center pixel numbered from 1 center X rotation center pixel numbered from 1 numbered from 1 yc Y rotation center pixel numbered from 1 scale enlargement factor subst substitution value Log book results E 38 options 0 simple shift 1 inversion 2 rotation shift scale 3 superposition 0 no 1 yes 0 no 1 yes 0 no 1 yes Excepted the text of the macro and the ending execution message the following information is recorded for instance in the case oper 3 file CI ADHOCW HELP adwt1b11 htm 3 of 4 15 02 02 09 34 43 294 000000 445 000000 340 000000 0017 01 Lower 21 33 23 Coordinates 0 to be modified 171 000000 ref 190 000000 144 000000 0017 01
138. 2 03 call 4 ad2 04 63115 ad 05 call 6 ad2 HOB call 7 ad2 08 call 4 ad 09 cal20 ad2 10 cal21 ad2 11 cal22 ad2 12 cal23 ad2 13 cal24 ad2 14 cal25 ad2 15 cal26 ad2 j 4 ar LS PPS horizontal cut 11 238 122242 c1 160 c2 210 minimum width is 7 41 pixels for file 04 measured widths file C ADHOCw HELP adwt1_h4 htm 2 of 4 15 02 02 09 34 59 ADwT1 tuning DEEE ET EEE TS This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example Macro TUNE_INSTR format 3 mode 0 linel 240 line2 240 col1 160 col2 210 F1 D Data Godbout call2 ad2 f2 D Data Godbout cal13 ad2 F3 D Data Godbout call4 ad2 f4 D Data Godbout cal15 ad2 F5 D Data Godbout cal16 ad2 f6 D Data Godbout cal17 ad2 Ff7 D Data Godbout cal18 ad2 f8 D Data Godbout cal19 ad2 F9 D Data Godbout cal20 ad2 10 D Data Godbout cal21 ad2 f11 D Data Godbout cal22 ad2 12 D Data Godbout cal23 ad2 Ff13 D Data Godbout cal24 ad2 14 D Data Godbout cal25 ad2 F15 D Data Godbout cal26 ad2 keyword content options TUNE_INSTR INSTR po ADA 2 bytes 1 ADA 4 bytes format data format 2 ADA 8 bytes 3 AD2 4 FITS mode type of analysis 0 horizontal cut 1 vertical cut 2 box
139. 2 15 02 02 09 33 43 ADw what is ADHOCw ADHOCw Return to main ADHOCw menu What is ADHOC ADHOC is a free software developed by the Interferometry Group of Marseille s Observatory ADHOC is the main software developed and used by the Interferometric Group of Marseille s Observatory to reduce the 3D data coming from Photon Counting or CCD observations It contains also general 2D modules useful for simple imagery It is commonly used to reduce CIGALE TIGER and PYTHEAS observations ADHOC is the acronym for Analyse et D pouillement Homog ne des Observations Cigale ADHOC software has been designed in 1987 in order to reduce data from the scanning P rot Fabry instrument CIGALE build in Marseille s Observatory Up to 1998 the successive versions of ADHOC run on DOS operating systems Since 1998 the software migrated to Windows environnement ADHOC is able to reduce data from a number of large telescopes 3m60 CFHT Hawaii 3m60 ESO Chile 1m50 ESO Chile 6m SAO Russia 1m93 OHP France 2m60 Byurakan Armenia 2m San Pedro Martir Mexico 1m50 Bosque Allegre Argentina 1m60 Mt Megantic Canada In 2001 about 150 papers in international magazines with external referees could refer to ADHOC software ADHOC concept is to minimize the training time for users All the user interface is graphical and a very friendly and complete HTML help is available at every moment ADHOC software has been written by J BOULEST
140. 238 01 Lower 14 19 57 Shift correction 0238 01 Lower 14 19 57 Shift RV 95 92 0238 01 Lower 14 19 57 Beginning step 7 map 0238 01 Lower 14 19 58 Beginning step 8 test 0238 01 Lower 14 19 58 Max corr2 1 00 channels Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c1 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_c1 htm 6 of 6 15 02 02 09 34 17 ADwT1 figure C01 full size 0 ADw phase ADHOCw Phase compulavan Input 3D file calibration Output 2D file rough phase as test ID ADHOCws_plus BLAISOUS Phas_bru AD2 Choose file Output 2D file parabolic phase used for reductions D ADHOCws_plus BLAISOUS Phas_prb AD2 Choose file Output 2D file test sum of all the calibration channels Choose file ID ADHOCws_plus BLAISOUS Sum_cal AD2 Output 2D file test Radial Velocities from calibration D ADHOCwSs_plus BLAISOUS RY_cal AD2 Choose file Scanning parameters Interference order p 162 at Calibration line 6598
141. 34 37 AdwT1 extraction of a channel ADwT1 Return to main ADHOCw help Return to main ADwT1 help B02 Extraction of a channel from a cube u ADw extract channel ADHOCw Lxectactag G channel fram a cube Input 3D file cube Output 20 file channel image Choose file Channel number to extract f Use an execution mask Execute Help x Abort EX Store macro The user must only notify the input 3D cube the channel number numbered from 1 and the 2D output file which will contain the extracted channel The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD2 This function can use an execution mask When the execution mask doesn t allow the file C ADHOCw HELP adwt1_b2 htm 1 of 3 15 02 02 09 34 37 AdwT1 extraction of a channel operation the extracting value is set to a null value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example EXTRACT3D2D fin D ADHOCws_plus BLAISOUS Call da3 fout D ADHOCws_plus BLATSOUS call_ch8 AD2 chnl 8 r keyword content options EXTRACT8D2D fin cube 3D input file name with whole path fout channel 2D out
142. 393 temp 20 0 incli 2 642 Compute exact tilt for a filter y te N SSS XS SDSS Click on the filter label to blink the curve CRE TT TRIS AR IN file C ADHOCw HELP adwt1_h8 htm 3 of 6 15 02 02 09 35 02 ADwT1 Interference filters 7 WSIS E 7 AA 2 TAN 6560 TE Z 6610 First select the telescope or aperture ratio or mean inclination angle warning aperture ratio doesn t take in account any central obturation If necessary update the mean inclination value by pressing the update appropriate button Then select the object parameters from radial velocity z redshift or final observed wavelength If necessary update the wavelength value by pressing the update appropriate button Chose the temperature of the filter Chose the drawing scales transm max allows a selection of the largest transmission in order to get a clearer drawing The press execute To display or not a filter toggle by clicking in the name box of the filter the curve will disappear and reappear Night sky spectrum is displayed in the bottom One possibility is to tilt filters to fit correctly with the observed wavelength This can only be used when the filter wavelength corrected from temperature is larger than the wavelength of observation In this case press the button Compute exact tilt and then after setting the observed wavelength and or filter name press Execute computation Res
143. 5 02 02 09 34 12 ADw3D main 2D display screen Profile displayed in zoom or image when you move the mouse the content of the pointed pixel can be displayed in the upper screen box A scrolling box allows to choose the 3D memory to display interferograms or wavelength maps Save 2D image allows to save the displayed image in a AD2 file Load 2D image allows to load the image from a AD2 file Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_b htm Return to main ADHOCw menu Return to main ADw3D menu file CI ADHOCW HELP adw3d_b htm 3 of 3 15 02 02 09 34 12 ADw3D full size main 2D Cube dimensions Ik 1512 ly 1512 lz 127 Mouse profile area fist pix v By Printer setup B Print screen Fac gy save data LabelBidon 7 Help 1 a Waiting gap sec Fan 19019 nivale General Statistics Phase Sum Interferograms Wavelength maps Mono cont RY Active the real time sum of interferograms Display parameters Graph area Compute sum again ixci2 gd 7 d re Display a channel fi im Inter
144. 5 1 32008 channel 3 12021 3 44743 channel 4 09088 8 57343 channel 5 122 0 80933 channel 6 A 3171 25 1309 channel 7 12815 6 2909 channel 8 13113 0 61405 channel 9 13371 3 63261 channel 10 11665 9 04831 channel 11 13577 1 65893 channel 12 15127 14 3795 channel 13 13752 5 79438 channel 14 11763 0 385923 channel 15 12283 2 60604 channel 16 10087 7 44292 channel 17 12475 2 49183 channel 18 0783 8 80247 channel 19 12844 4 93185 channel 20 14931 3 25755 channel 21 213573 2 55281 channel 22 10161 6 69087 channel 23 12803 1 88395 channel 24 0461 6 3895 channel 25 14096 4 88995 channel 26 15071 7 95798 channel 27 A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B A and B for Y AX B file C ADHOCw HELP adwt1_c5 htm 9 of 11 15 02 02 09 34 46 ADwT1 photometry from OH A you see there are strong variations of the transparency which varies as A and of the sky background which varies as B
145. 5 truc adp nbdim 2 x1 1 x2 256 stepx 2 modex 1 yl 1 y2 128 stepy 4 modey 1 keyword content options SUB_ENTITY fin 3D input file name with whole path fouts 3D output file name created in the new directory a output parameters file name created in the new directory nbdim Inbdim nb of dimensions 2 image or 3 cube _ or 3 2 image or 3 cube _ X1 starting X coordinate X2 ending X coordinate stepx spacing between 2 X samplings file C ADHOCw HELP adwt1b10 htm 3 of 5 15 02 02 09 34 31 ADwT1 sub subes or images modex X sampling mode individual sampling binning yl starting Y Starting Y coordinate starting Y coordinate ending Y coordinate stepy spacing spacing between 2 Y samplings 2 Y samplings pacing between Ysamplings modey Y sampling mode individual sampling binning zis zi starting Z Starting Z coordinate only if nbdim 3 only if nbdim 3 starting Z coordinate only ifnbdim 3 si Z2 ending Z coordinate only if nbdim 3 stepz spacing spacing between 2 Z samplings only if nbdim 3 2 Z samplings only if nbdim 3 Spacing between 2 2 samplings only fnbdim 8 modez Z sampling mode only if nbdim 3 individual sampling i binning Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulest
146. 6 G016 adt fout D M31_GHASP bidon ad3 cycle dep 1 cycle_end 3 norm 1 reman 1 rempix 0 parasit 1 sigma_parasit 5 keyword content options EXTRACT3D2D ifin frames ADT input file name with whole path fout cube 8D output file name with whole path o file C ADHOCw HELP adwt1_e1 htm 3 of 5 15 02 02 09 34 06 ADwT1 ADA IPCS integration cycle dep departure cycle number numbered from 1 cycle cycle_end yele_ende_ ending cycle number numbered from 1 norm frame count normalization mode 0 no 1 yes reman correction of remanence no A yes rempix delta x delta y difference of location for remanence 0 same pixel in pixels if reman 1 1 3x3 pixels 2 5x5 pixels 3 7x7 pixels parasit cameo external TV parasites no yes sigma _ sigma_parasites frame count frame count accepted under mean sigma_ parasites under mean sigma_ frame count accepted under mean sigma_ parasites Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0003 01 Lower 18 31 07 Huge memory global cube allocated 0003 01 Lower 18 31 10 Initializing the 3D array 0003 01 Lower 18 31 10 3D array initialized 0003 01 Lower 18 31 10 moy sig discri 8 9 5 6 37 0003 01
147. 9 33 54 ADw2D 3D profiles Chnl offset allows to shift in X the profile for P rot Fabry profiles modulo in order to display the maximum of the line at a convenient location Default Chnl offset value is 0 Positive and negative values are accepted Intens offset the profile is shift in Y in order to separate the different profiles coming from other 3D files The offset value is simply added to the origin value for display Default Intens offset value is O When switching to the Image folder the windows becomes the following The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page ADIINCGw D disping nn ADC raniewt 22 iva wesmex CONTE Shane SS Cic c spay LAr P exp eine Min a socal sete 7 He af x Wa th gt peace do ke 20231 H HA 6 LI annleis fi t1 gt B aa ta gt Pases Irago Main imag Mana ORG AN S dem DEC D inhar Wo sone Dipy ja dnx NES salwe F Irssi c pills RL LE T Fih sia th Inap vel toe bates Ut Tobe rake i il abo Ct erstics Hosier Hara litara a l A ri XKKO Had 2 CLC r a h 3 dus tye th F4 ats si pind i exch ies hon 2I As H f p TS Hud F Te i te Ds Wade a RL A Ce 27 cuz ha ion dit 1 p lt 5 4 s moe itikuti wil 10 orbs ESE Pois em if
148. 9 34 50 ADwT1 mixing ADS seeing files O oO O oO O O O oO O oO O oO O O O oO O oO O oO O oO O oO O oO O O O oO O oO O oO O O O oO O oO O n H FH FH FH FH FH He OU H FH OU FHV FH He OU OU H FH HE OU FH FH HTH FH H F HH U O 0 D D ND D ND D NN D NN D N D NO ND D ND D ND D ND D ND D ND D ND D ND D ND D N D N D N D ND D ND D ND D ND D N oO eeing 2 256759 pixel 0 01 Iower 09 2 eeing 1 954411 pixel 0 01 Iower 09 2 ing 2 523134 pixel 0 01 Iower 09 2 ing 2 256759 pixel 10 01 Lower 09 2 ing 2 256759 pixel 10 01 Lower 09 2 ing 2 523134 pixel 10 01 Lower 09 2 ing 2 523134 pixel 10 01 Lower 09 2 ing 2 523134 pixe 0 01 Iower 09 2 ing 2 523134 pixel 0 01 Iower 09 2 ing 2 256759 pixel 10 01 Lower 09 2 ing 2 256759 pixe 10 01 Lower 09 2 ing 2 256759 pixe 10 01 Lower 09 2 ing 1 595770 pixel 10 01 Lower 09 2 ng 2 523134 pixel Q 01 Lower 09 2 ing 1 954411 pixel 10 01 Lower 09 2 ing 1 954411 pixe 10 01 Lower 09 2 ing 1 954411 pixel 10 01 Lower 09 2 ing 2 256759 pixel 10 01 Lower 09 2 ing 1 954411 pixel 10 01 Lower 09 2 ing 1 954411 pixel 10 01 Lower 09 2 ing 1 954411 pixe 10 01 Lower 09 2 ing 1
149. 9 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 22 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 24 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 24 F02 TIGER CUBE Info 0134 16 Batch Lower 16 24 24 F02 TIGER_CUBE Info Opening and creating miscellaneous files Reading selected spectra Nb of input selected spectra 547 Reserving arrays Longer selected spectra 59 pixels Nb of input calibration lines 2 Wavelength 0 6532 882 A Wavelength 1 6598 953 A Integrating calibration spectra Rejected coordinates of spectra from sigma dispersion Position sigma of lines 1 2 1 72088 pixels 80 x1 113 y1 85 x2 183 y2 89 deviation 9 5 pixels 232 x1 19 y1 224 x2 81 y2 228 deviation 8 7 pixels 327 x1 21 y1 307 x2 91 y2 311 deviation 8 7 pixels 395 x1 568 y1 368 x2 639 y2 372 deviation 10 9 pixels 419 x1 378 y1 389 x2 455 y2 393 deviation 10 0 pixels Nb of rejected spectra from sigma position 5 Nb of remaining calibrated spectra 542 Rejected coordinates of spectra from intensity dispersion Output cube dimensions 53 26 181 Reference origin position in output frame 25 12 Nb total of object measured spectra 951 Nb total of calibration verification measured spectra 951 Saving eventual ADH Pytheas file Correct end Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1_f2 htm 7 of 8 15 02 02 09 34 33 ADwT1 TIGER 2 Note all ADHOCw help is
150. 953 Calibration scan 6598 953 6562 780 Angstroems Object line 6562 780 Object scan 6571 640 Object RY 0 00 Modify these parameters Helioc RY correct file C ADHOCw HELP ADwT1C1t htm 15 02 02 09 34 18 Wavelength of the channel H 6560 000 Angstroems Load Mid spectrum 6560 000 A Load Calibration 6598 953 A Geometry Center of rings Xe 257 50 Ye 262 50 Pixel ratio X 1 00000 F X forced to 1 CCD Compute and check coherence of center and ellipticity Enforce the given values ot center and ellipticity 2D including mask x1 f yi fi x2 512 y2 512 l More complex execution mask lel Es Selective sector __ angle min 0000 angle max 360 000 R max 9999 00 Profiles measurement Slope recommended k Hb of chnis C Fixed levels 20 lle 9 o E Store macro Help V4 Execute X Abort Eh store mecro __ w A teue __ Am ADwT1 translation of the phase to old ADHOC format ADwT1 Return to main ADHOCw help Return to main ADwT1 help H02 Translation of a parabolic phase into an old ADHOC DOS phase ADw translate phase Miel ADHOCw 7ransiating phase te old APHOC DOS Input 20 file parabolic phase ADHOCws plus BLAISOUS Phas_prb AD02 Choose file Output 20 file fold ADHOC phase Choose file D ADHOCwS plus BLAISOUS Phas _org DA2 Stor
151. 954411 pixel 10 01 Lower 09 2 ing 1 595770 pixel 10 01 Lower 09 2 ing 1 595770 pixe 10 01 Lower 09 2 ing 1 595770 pixe 10 01 Lower 09 2 file C ADHOCw HELP adwt1_c7 htm 4 of 5 15 02 02 09 34 50 WA WHA WN WN WHA WHA WHA WA WHA UNUN WUU WHA WHA WHA WA WHA UU WH WHA WHA WHA WA WHA WN W U Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch an an an an an an an an an an an an an an an an an an an an an an an an 2 3 4 5 6 7 1 8 9 dx 0 118500 dy 0 226305 dx 0 344532 dy dx 0 390465 dy dx 0 186344 dx 0 967372 dx 2 614692 dx 2 529139 dx 2 424751 L 197466 L 252195 dy 1 025478 dy 0 673867 dy 2 003112 dy 2 725814 dy 3 098307 10 dx 2 262654 dy 2 747652 an 20 21 22 23 24 25 26 dx 2 162074 dx 1 501220 dx 1 625759 dx 1 236128 dx 1 319715 dx 0 994150 dx 1 389092 dx 1 366964 dx 1 977035 dx 1 329942 dx 1 642878 dx 1 733310 dx 1 847989 dx 1 785484 dx 2 049300 dx 0 956918 dy 2 dy 2 dy 0 dy 1 dy 0 dy 0 dy 0 dy 1 dy 0 dy dy dy dy dy dy dy 273902 094481 967323 128864 939947 901245 950727 1
152. 99452 0 channel 29 A and B for Y AX B 999848 0 channel 30 A and B for Y AX B 999843 0 channel 31 A and B for Y AX B 99983 0 channel 32 A and B for Y AX B 999795 0 channel 33 A and B for Y AX B 999666 0 channel 34 A and B for Y AX B 999642 0 channel 35 A and B for Y AX B 999672 0 channel 36 A and B for Y AX B 999624 0 channel 37 A and B for Y AX B 99956 0 channel 38 A and B for Y AX B 99959 0 channel 39 A and B for Y AX B 999564 0 channel 40 A and B for Y AX B 999628 0 channel 41 A and B for Y AX B 999528 0 channel 42 A and B for Y AX B 999591 0 channel 43 A and B for Y AX B 999565 0 channel 44 A and B for Y AX B 99947 0 channel 45 A and B for Y AX B 999516 0 channel 46 A and B for Y AX B 999471 0 channel 47 A and B for Y AX B 999461 0 channel 48 A and B for Y AX B As expected on the contrary of C05 function output B is always zero with C11 function Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1c11 htm 7 of 8 15 02 02 09 34 53 ADwT1 rough photometry Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the
153. A and B values null else 8 gt F3 F1 if F2 is outside A and B values null else 9 gt F3 F1 if F2 is inside A and B values F2 else 10 gt F3 F1 if F2 is outside A and B values F2 else 11 gt F3 F2 if F2 is inside A and B values F1 else 12 gt F3 F2 if F2 is outside A and B values F1 else floating variable used in the operation floating variable used in the operation floating variable used in the operation Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0252 01 Lower 11 50 34 Files are 3D F1 amp F2 input F3 output 0252 01 Lower 11 50 34 Operation F3 A Fl B F2 C file C ADHOCw HELP adwt1_b6 htm 4 of 5 15 02 02 09 34 39 ADwT1 masking operations 0252 01 Lower 11 50 34 with a 1 000000 b 1 000000 and c 0 000000 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b6 htm Return to main ADHOCw menu Return to main ADwT1 menu file C AD
154. A and B for Y AX B 13496 5 68456 channel 25 A and B for Y AX B 13539 5 70234 channel 26 A and B for Y AX B 13764 5 79859 channel 27 A and B for Y AX B You see here that A and B are now almost constant The photometry is within 1 The reason why A and B are not exactly 1 0 and 0 0 is due to the fact that the summed reference profile is not exactly the mean profile but it doesn t matter the result is extremely satisfactory Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1_c5 htm 10 of 11 15 02 02 09 34 46 ADwT1 photometry from OH Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c5 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_c5 htm 11 of 11 15 02 02 09 34 46 ADHOCv Typical reduction procedure ADHOCw Return to main ADHOCw menu A typical reduction procedure for CIGALE observations Difference of reduction between CCDs observations and photon counting IPCS observations The CCD data reduction is more complex than the IPCS one because the user must correct fro
155. ADHOC software ADHOCW sottware for Windows 32 bits Observatoire de Marseille France Analyse et D pouillement omogene des Observations Cigale ADHOCw ADHOC is the main software used by the Interferometric Group of Marseille s Observatory to reduce the 3D data coming from Photon Counting or CCD observations It contains also general 2D modules useful for simple imagery ADHOC is the acronym for Analyse et D pouillement Homog ne des Observations Cigale ADHOC software has been designed in 1987 in order to reduce data from the scanning P rot Fabry instrument CIGALE build in Marseille s Observatory Up to 1998 the successive versions of ADHOC run on DOS operating systems The new version will offer also to reduce TIGER and PYTHEAS observational data ADHOC was able to reduce data from a number of large telescopes 3m60 CFHT Hawaii 3m60 ESO Chile 1m50 ESO Chile 6m SAO Russia 1m93 OHP France 2m60 Byurakan Armenia 2m San Pedro Martir Mexico 1m50 Bosque Allegre Argentina 1m60 Mt file C ADHOCw HELPiindex html 1 of 3 15 02 02 09 33 42 ADHOC software Megantic Canada About 100 papers in international magazines with external referees could refer to ADHOC software ADHOC concept is to minimize the training for the users All the user interface is graphical and a very friendly and complete HTML help is available at every moment ADHOC software has been written by J BOULESTEIX Observato
156. ADHOCw Unix AD3 swapped float32 by channels inputtype for 2D files 0 ADHOCw default AD2 float32 1 ADHOC old VISU2 DA2 int16 2 not used 3 FITS any type float32 float64 int8 int16 int32 4 not used 5 not used 6 Binary or IDL PC int16 7 Binary or IDL PC float 8 not used 9 not used 10 Binary or IDL Unix int16 11 Binary or IDL Unix float 12 23 not used outputtype for 2D files 0 ADHOCw default AD2 PC float32 1 ADHOC old VISU2 DA2 PC int16 2 not used 3 FITS 32 float32 4 not used 5 not used 6 Binary or IDL PC int16 7 Binary or IDL PC float 8 not used 9 not used 10 Binary or IDL Unix int16 11 Binary or IDL Unix float 12 not used 13 not used 14 FITS 64 float64 15 not used 16 FITS 8 int8 17 not used 18 FITS 16 int16 19 not used 20 FITS 32 int32 21 not used file C ADHOCw HELP adwft_d htm 4 of 6 15 02 02 09 34 09 ADwFT Macros and batch 22 ADHOCw AD2 Unix swapped float32 Warning1 Possible error for 3D gt 2D_ slices or 2D_slices gt 3D conversions The inputtype and outputtype for slices must be as 2D inputtypes or 2D outputtypes Usual error is to give inputtype or outputtype for slices as 3D ordered by channels This leads to a runtime error Warning2 Ix ly and nc parameters are OBLIGATORY for slice operations any comment Warning 1 Don t forget the at the end 2 a space at least must
157. ADHOCw HELP adwft_d htm 6 of 6 15 02 02 09 34 09 ADw3D general functions ADw3D Return to main ADHOCw help Return to main ADw3D help General functions These functions appear on the upper part of the window and are available for any folder Cube dimensions x B12 ls BE E 27 Printer setup Print screen S Save 30 data Help Quit the program Printer setup choose printer and orientation i Wating gap sec Print screen print the window on the current Window printer Save 3D data copies the 3D current cube onto a 3D AD3 file Help get ADw3D help Save to BMP save the current folder image to a BMP image file In addition the user may also save the scale as BMP image file file C ADHOCw HELP adw3d_e htm 1 of 2 15 02 02 09 34 10 ADw3D general functions Quit the program quit ADw3D Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_e htm Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_e htm 2 of 2 15 02 02 09 34 10 ADw3
158. AORC 20231 i HA Se LI anuli fi 11 gt ss ta Perses Irsge wiadin b 4414 het un 14 lu nlg mhk ikqale ou ba que LT F whe z Il 11 Hu Fh He Lace Sung ri Fh HE Ewwel su Fh HH Lire EVE eu Fk HE Lawe Susp it Fh HE z Nise Fhe Vitk Cki Diang Class es Hamra zair Jscl gzord Faust Loin Zulofse Imens ches peur mtk El wr i gt 7 ced r fi rivu 7 ro r f fe L ly Visible if No the profile will not be displayed and modifications will not be allowed Color color of the profile drawing 16 basic colors available Drawing direct means that the color is displayed like this complementary will display at any pixel the complementary color with the 2D image background color Cell indicated the square side of the profile integration for instance 3 will integrate 9 pixels 5 will integrate 25 pixels Normalization individual if the profile is normalized in every cell global if the Y scale of the profiles are identical for all the cells and normalized on the largest one Background yes or no indicate if the background must be drawn or not If not all the profiles are substracted from the lowest value of the channels First chnl and Last chnl allow to display only channel in a limited range It is like a zoom in X As default First chnl is set to 1 and Last chnl to the maximum channel number file C ADHOCw HELP adwa2d_e htm 2 of 8 15 02 02 0
159. ASCII text editor 4 IDL and binary formats These formats are extremely simple The 2D or 3D arrays are written in binary 4 types of data formats are available integers 2 floats 4 swapped integers 2 from Unix swapped floats 4 from Unix Swapped UNix mode has 4 rules bytes and not bits are swapped short int 16 values are looked in 4 bytes blocks byte 1 ab and byte 2 cd are abcd 4 bytes blocks 2 int16 1 int82 or 1 float32 are swapped like this abcd gt dcba characters strings for instance comments are not swapped Example of program in Fortran for 2D images and integers 2 and floats 4 integer 2 itab 50 dimension tab 50 Ix 50 ly 50 c opening output files open unit 21 file int idl access direct recl Ix 2 status unknown open unit 22 file float idl access direct recl Ix 4 status unknown c array initialization do 1 i 1 Ix itab i i tab i i 1 continue c writing the 2D data pixel file C ADHOCw HELP adw_what htm 10 of 15 15 02 02 09 33 45 ADw what is ADHOCw do 11 j 1 ly write 21 rec j itab i i 1 Ix write 22 rec j tab i i 1 Ix 11 continue c closing files close 21 close 22 end Example of program in Fortran for 3D cubes and integers 2 and floats 4 integer 2 itab 50 60 dimension tab 50 60 Ix 50 ly 60 Iz 24 c opening output files open unit 21 file int idl access direct recl Iz 2 status unk
160. AS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info file C ADHOCw HELP adwt1_g1 htm 12 of 14 15 02 02 09 34 36 buffering spectra 481 500 buffering spectra 501 520 buffering spectra 521 540 buffering spectra 541 547 Step 4 building the 3D Computing line 1 53 Computing line 2 53 Computing line 3 53 Computing line 4 53 Computing line 5 53 Computing line 6 53 Computing line 7 53 Computing line 8 53 Computing line 9 53 Computing line 10 53 Computing line 11 53 Computing line 12 53 Computing line 13 53 Computing line 14 53 Computing line 15 53 Computing line 16 53 Computing line 17 53 Computing line 18 53 Computing line 19 53 Computing line 20 53 Computing line 21 53 Computing line 22 53 Computing line 23 53 Computing line 24 53 Computing line 25 53 Computing line 26 53 Computing line 27 53 Computing line 28 53 Computing line 29 53 Computing line 30 53 Computing line 31 53 Computing line 32 53 ADwT1 PYTHEAS 1 0182 16 Batch Lower 18 42 24 G01 0182 16 Batch Lower 18 43 50 G01 0182 16 Batch Lower 18 45 17 G01 0182 16 Batch Lower 18 46 36 G01 0182 16 Batch Lower 18 47 51 G01 0182 16 Batch Lower 18 49 07 G01 0182 16 Batch Lower 18 50 26 G01 0182 16 Batch Lower 18 51 45 G01 0182 16 Batch Lower 18 52 23 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower 18 52 27 G01 0182 16 Batch Lower
161. C But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_gf htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_gf htm 4 of 4 15 02 02 09 34 29 ADwT1 function menu window ADwT1 Return to main ADHOCw help Return to main ADwT1 help Function menu window When the program runs two windows appear the function menu window and the task manager window At any time each one of the windows can be brought to front by pressing the buttons Bring task manager to front or Bring general menu to front ADwT1 Pytheas a ioj x Hide task manager window Version l Bring task manager to front AD H OCw ADwT1 2001E JBx Obs Marseille l 1280 x 1024 96 ppi General 2D 3D operations Cigale Profiles 1Pcs Tiger Pytheas Miscell Ot COMMING 2D POCA man Compute wavelength 3D maps Compute monochromatic continuum radial velocities line widths 2D maps EA Edit a batch file 4 Substract OH and or continuum from given areas pe Get photometric parameters from OH lines case of CCD gt ADX file ix Exec a batch file Get seeing analysis channel channel case of CCD gt ADS file Merging of several ADS seeing parameters files Photometric corre
162. CWs_plus BLAISOUS Zones_oh adz flbmp Jbx_portable D ADHOCWs_plus BLAISOUS OH BMP ftxt Jbx_portable D ADHOCWs_plus BLAISOUS OH TXT mode_ref 0 nbpass 1 fact1 1 000000 mode_cont 0 mode_prof 1 file C ADHOCw HELP adwt1_c4 htm 4 of 6 15 02 02 09 34 15 ADwT1 OH and or continuum substraction fprof Jbx_portable D ADHOCWs_plus BLAISOUS PROFILOH AD1 keyword content options SUBSTRACT_OH OH ee to insert 2D input file name with whole path fout cube to modify 3D output file name with whole path fzones zones ADZ ADZ area coordinated ASCII file ADZ area coordinated ASCII file ASCII file mode_ref reference mode no a reference file 2D reference file SE in fref fref 2D 2D reference image file if mode_ref 1 2D reference image file if mode_ref 1 file if mode_ref 1 ee SE a 1 to 3 default is 1 facti substraction factor for passt defaultist fact2 substraction factor for pass 2 if nbpass gt 1 fact3 substraction factor for pass 8 if nbpass gt 2 mode cont substraction of continuum 0 no 1 total substraction at last pass 2 partial substraction at last pass value cont mm cont continuum to substract if mode_cont 2 Log book results Excepted the text of the macro and the ending execution message the following information is recorded for instance in the case oper 3 0019 01 Lower 22 13 11 Zone 1 x1 100 000
163. Ch Ch Ch Ch Ch Ch Ch Ch Ch Ch an an an an an an an an an an an an an an an an an an 1 2 3 4 5 6 7 8 9 dx 1 324298 dy 0 766408 dx 0 118500 dy 0 226305 dx 0 344532 dy 1 197466 dx 0 390465 dy 1 252195 dx 0 186344 dy 1 025478 dx 0 dx 2 dx 2 dx 2 967372 dy 0 673867 614692 dy 2 003112 529139 dy 2 725814 424751 dy 3 098307 10 dx 2 262654 dy 2 747652 an dx 2 162074 501220 625759 236128 col 9715 994150 389092 366964 977035 dy 2 dy 2 dy 0 dy 1 dy 0 dy 0 dy 0 dy 1 dy 0 273902 094481 967323 128864 939947 901245 950727 100537 879370 ADwT1 seeing analysis 0210 O1 Lower 09 23 20 Channel 20 dx 1 329942 dy 1 447687 seeing 1 954411 pixels 0210 O1 Lower 09 23 20 Channel 21 dx 1 642878 dy 1 560732 seeing 1 954411 pixels 0210 0O1 Lower 09 23 20 Channel 22 dx 1 733310 dy 1 513467 seeing 1 954411 pixels 0210 O01 Lower 09 23 20 Channel 23 dx 1 847989 dy 1 678005 seeing 1 595770 pixels 0210 O1 Lower 09 23 20 Channel 24 dx 1 785484 dy 1 791716 seeing 1 595770 pixels 0210 O1 Lower 09 23 20 Channel 25 dx 2 049300 dy 1 576296
164. Cw parameters file ADP D poullement Create a new ADHOCw parameter file ADP be nest Lt Execute create modify a global macro batch ADB command file Cigale indonus 32bits Help X Abort This program requests a minimum screen of 800x600 with 16 colors If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode An ADP parameters file is absolutely necessary for the data processing This file has a similar function with the param cig files in the old ADHOC DOS software file C ADHOCw HELP adwt1_ge htm 1 of 3 15 02 02 09 33 46 ADwT1_gene You can open an already existing ADP parameter file or create a new one When an ADP file exists it can be changed at every moment by using the A01 function of the ADwT1 program Note that the ADHOC software manages completely the Windows networks you can access and write if permitted by the manager to any data file located on another computer All the files are completely shared in reading but locked only to one writing user at the same time ADHOC ADwT1 can run Simultaneously 16 different tasks including a unique batch task But several ADHOCw ADwT1 programs can run simultaneously in different directories Important note The ADwT1 assumes that the Z size of the cubes wavelength dimension is covering completely an interference order i e a not
165. D ADHOCws_plus BLATSOUS Cont_ORG AD2 frv D ADHOCws_plus BLAISOUS VR_ORG AD2 fwidths D ADHOCws_plus BLATSOUS Width_ORG AD2 mode_emiss 0 algorithm 1 chg_chnls 2 cont 2 keyword content options MONORV fin BD input file name with whole path dephased cube fmono 2D output file with whole path rough phase PO fcont 2D output 2D output file with whole path parabolic phase 2D output file with whole path parabolic phase whole path parabolic phase eo o 2D output file with whole path sum of the calibration channels fwidths 2D output file with whole path radial velocity of the calibration through the parabolic phase mode_emiss emission or absorption 0 emission 1 absorption algorithm algorithm to analyze the profile slope change fixed levels chg_chnls number of successive inversed channels in case of see Note 1 algorithm 1 pc_mono percentage of measured channels in case of eae Not algorithm 2 cont mode to compute continuum 1 percentage of channels 2 mean of the 3 lowest channels 3 value of the lowest channel pc_cont percentage of measured channels for continuum only if cont 1 Note 1 chg_chnls and pc_mono exclude themselves Log book results Excepted the text of the macro and the ending execution message no information is recorded file C ADHOCw HELP adwt1_c3 htm 3 of 4 15 02 02 09 34 52 ADwT1 monochromatic co
166. D ADwT1 ADwWFT or ADWIPCS if the screen definition is not sufficient But you can work nevertheless in reduced display mode If the screen size is smaller than required you will need to use the scrollbars on the right and bottom sides of the window to access to the whole window If the number of colors is smaller than required the displayed colors can be affected If the Pixel per Inch value is not 96 the best is to change it now if not the graphics and the text could be largely distorted sometimes unreadible To change the Pixel Per Inch value go to the Control Panel and then to the Display ions of the Window system Put the fonts to small fonts instead of large fonts file C ADHOCw HELP adw_scr htm 2 of 4 15 02 02 09 33 47 ADw screen warning Recommended parameters for the different ADHOCw programs ADw2D 2Ddisplay program 1024768 256 9 ADw3D 3D display program I280x1024 256 96 ADwTi data reduction program 800x600 16 9 ADWFT file translation program 640x480 16 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhoc
167. D main 3D display screen ADw3D Return to main ADHOCw help Return to main ADw3D help This mode corresponds to the Interferograms folder The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens to visualize the figure with full resolution for help manual on paper see next page Er NES U display mun panci C bain E F t e He z CERN des LENS iat Aro FB Ex Dds p TE OPR ECG 2 SE ai eee L TF EE He sed all les se CES Lane tes gel im ete vers i T S He ANG Lho e LEP iagh man Ie z sw Ezy xi yi 133 iis file C ADHOCw HELP adw3d_a htm 1 of 4 15 02 02 09 34 10 ADw3D main 3D display screen ES Display parameters Graph atea 256x256 Image area 51 2x512 xo YO hm iz Zoom in mouse right button Zoom out shift mouse right button fa ainbow v Scale max 16160 Threshold 1 1 10 10 100 5 cale min O Scale overlap amp Load a new 3D ft re Actualize display Page folders You can access to two pages folders Interferograms this 3D display and Sum 2D display Here the folder is Interferograms file C ADHOCw HELP adw3d_a htm 2 of 4 15 02 02 09 34 10 ADw3D main 3D display screen Zoom The image area can be easily zoomed The simplest way is to click on the right button on the mouse it will be a zoo
168. DV array for velocity curves Create a regular array with following parameters Crowns pixels 20 Systemic velocity Kms 2320 00 This option gives the possibility to fill a large number PA w t top degrees 35 00 Inclination w r sky degrees 20 00 of cells before modifying them manually Half sector degrees 20 00 R min pixels 128 00 R max pixels 128 00 Suppress line gt fi Insert a new line R RUEE fine gt afi f Clear array J Help ee En PO De LP a A Acquire array amp go to image 110 00 15 00 55 00 2320 00 30 00 eT 100 00 15 00 55 00 2320 00 30 00 Huk ut reading array 90 00 15 00 55 00 2320 00 30 00 80 00 15 00 55 00 2320 00 30 00 Notes 1 70 00 15 00 55 00 2320 00 30 00 Rmin and Rmax are in pixels f on the sky 60 00 15 00 55 00 2320 00 30 00 PAR ani PASSE wie hi 50 00 15 00 55 00 2320 00 30 00 degrees with respect to the top of the image and counted J 40 00 15 00 55 00 2320 00 30 00 in direct sense inverse 30 00 15 00 55 00 2320 00 30 00 clockwise Vs is in km s 20 00 15 00 55 00 2320 00 30 00 incli is in degrees with 10 00 15 00 55 00 2320 00 30 00 resect tothe sty plane 0 00 15 00 55 00 2320 00 30 00 Note 2 10 00 18 00 58 00 2320 00 30 00 It is recommended to have crowns increasing radii in 20 00 21 00 61 00 2320 00 30 00 order to get a correct drawing an nn 24 nn Rann o20n nn an nn of the sectors the drawing of file JIICVADHOCW HELP adw2d k2 htm
169. DwFT allow batches Batches are operations macros which are stored in advance in an ASCII file in order to be sequentially executed later ADWT1 macros are very easy to create after filling the parameters box of a given function you can choose either to execute immediately the function by pressing the Execute button either to write append the macro code onto a batch macro ADM ASCII file by pressing the Store macro button The main ADwT1 menu allows you to run a batch macro ADM file instead of a function by pressing the Exec a batch file button The macros have a simple syntax a code operation and parameters as examples show it Macro comment lines are allowed The file in which macros can be stored is an ASCII file of ADM suffix AHOHCw macro This ADM file can be edited easily by the user in order to generate new sequences In addition it is possible to chain different ADM macro files defined in different directories in a global macro batch ADB file Null values Null values are values which are not displayed and not taken in account during computations for example pixels without valid measure 2D and 3D files can have null values For files containing floating values new ADHOC floating FITS the null value is 3 1E 38 All values less than 3 0E 38 are considered as null For files containing integer values old ADHOC integer FITS the null value is 32768 All values less than 32000 are considered as null file
170. EAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info file C ADHOCw HELP adwt1_g1 htm 11 of 14 15 02 02 09 34 36 buffering spectra 61 80 buffering spectra 81 100 buffering spectra 101 120 buffering spectra 121 140 buffering spectra 141 160 buffering spectra 161 180 buffering spectra 181 200 buffering spectra 201 220 buffering spectra 221 240 buffering spectra 241 260 buffering spectra 261 280 buffering spectra 281 300 buffering spectra 301 320 buffering spectra 321 340 buffering spectra 341 360 buffering spectra 361 380 buffering spectra 381 400 buffering spectra 401 420 buffering spectra 421 440 buffering spectra 441 460 buffering spectra 461 480 ADwT1 PYTHEAS 1 0182 16 Batch Lower 18 17 30 G01 547 0182 16 Batch Lower 18 17 32 G01 547 0182 16 Batch Lower 18 17 33 G01 547 0182 16 Batch Lower 18 17 35 G01 547 0182 16 Batch Lower 18 17 35 G01 output file 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower 18 17 35 G01 0182 16 Batch Lower
171. EIX Observatoire de Marseille boulesteix observatoire cnrs mrs fr ADHOCw present version is working on Windows 32 bits systems 95 98 NT 2000 uses multi tasking and manages completely file sharing on networks Direct dialog or macros can be used There are no size limitations in the 3D dimensions of the data that ADHOCw can reduce ADHOCw works mainly on 4 bytes floating values witch offers a large dynamics for the data ADHOCw software is free of use and can be duplicated Information of the interest of users is welcome and a user list is maintained by boulesteix observatoire cnrs mrs fr who will inform regularly of the availability of the new releases ADHOCw ADHOC for Windows code source is written in C with the Borland C Builder tool using the classical Microsoft Windows primitives file C ADHOCw HELP adw_what htm 1 of 15 15 02 02 09 33 45 ADw what is ADHOCw ADHOCw allows simultaneous computations at the same time 16 simultaneous tasks maximum and on the same shared files ADHOCw accepts batch macros which can be easily edited by the users System and hardware requirements for the Windows version ADHOCw ADHOC for windows must run on Windows 32 bits operating systems Windows 95 98 Windows NT or Windows 2000 Executable code is compatible with Intel 80386 Intel 80486 Intel Pentium Intel Pentium Pro Intel Pentium Il Intel Celeron Intel Pentium Ill Intel Pentium IV AMD Duron AMD Althon a
172. ENYNONE array initialization for k 0 k lt lz k itab k k tab k k writing the 3D data profile for j 0 j lt ly j for i 0 i lt Ix i Iseek lu_int 2L Ix j lz i 1z SEEK _SET write lu_int itab 2L Iz Iseek lu_float 4L Ix j lz i lz SEEK_SET write lu_float tab 4L 1z closing files file C ADHOCw HELP adw_what htm 12 of 15 15 02 02 09 33 45 ADw what is ADHOCw close lu_int close lu_ float delete itab delete tab 5 FITS format ADHOCw File Translator accepts almost all of the FITS formats floats 32 and 64 integers 8 16 and 32 FITS was first developed in the late 1970 s as a standard data interchange format between various astronomical observatories Since then FITS has become the defacto standard data format supported by most astronomical data analysis software packages A FITS file consists of one or more Header Data Units HDUs where the first HDU is called the Primary HDU or Primary Array The primary array contains an N dimensional array of pixels such as a 1 D spectrum a 2 D image or a 3 D data cube Five different primary datatypes are supported Unsigned 8 bit bytes 16 and 32 bit signed integers and 32 and 64 bit floating point reals Any number of additional HDUs may follow the primary array these additional HDUs are called FITS extensions There are currently 3 types of extensions defined by the FITS standard
173. G 4140141993 18 08 57 d placements top lime fall scale 14 4385 Y displacements center aqual full scale 144385 Seeing variations bottom ired fullacale 17 5172 Comment or information file C ADHOCw HELP adwt1_di htm 2 of 3 15 02 02 09 34 15 ADwT1 control display Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_di htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_di htm 3 of 3 15 02 02 09 34 15 ADwT1 execution mask ADwT1 Return to main ADHOCw help Return to main ADwT1 help Execution mask Some functions can use an execution mask HO ADw execution mask als Es ADHOCw mask for execution Note limit values are 3 1638 and 3 1E38 Null value is 3 1E38 the rectangular area xclude the rectangular area Exclude nclude the channels k1 h k2 Pr bounds are included Note 19 6 is the inverse of 7 18 If k2 lt k1 channels from k2 to K1 through channel 1 are selected nclude the values 34E 38 1E 38 lt 3 1E 38 bounds are included se a 2D image mask M Use mask pixel will be sel
174. HIS IS NOT IMPORTANT because the seeing correction of the ADHOCw function C08 is relative So only the relative value of the seeing is important The user can easily mix different ADS files issued from different stars with different seeing The output ADS seeing parameter file is ASCII and has a special ADS format The output BMP file is similar with the ADHOCw function C06 one This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example MIX_SEEING f 1 E ADHOCws_plus BLAISOUS bidon ads fact1 1 000000 2 E ADHOCws_plus BLAISOUS bidon2 ads fact2 0 870000 3 E ADHOCws_plus BLAISOUS bidon3 ads fact3 1 450000 fseeing E ADHOCws_plus BLAISOUS toto ads file C ADHOCw HELP adwt1_c7 htm 2 of 5 15 02 02 09 34 50 ADwT1 mixing ADS seeing files fbmp E ADHOCws_plus BLAISOUS Seeing BMP keyword contet options MXSEEING Log book results Excepted the text of the macro and the ending execution message the following information is recorded 02 02 0O1 Lower 09 23 19 Total weight 3 320000 01 Lower 09 23 20 Channel 1 dx 1 324298 dy 0 766408 O 0 0 file C ADHOCw HELP adwt1_c7 htm 3 of 5 15 02 02 0
175. HOCw HELP adwt1_b6 htm 5 of 5 15 02 02 09 34 39 ADwT1 mixed arithmetic operations Return to main ADHOCw help Return to main ADwT1 help B07 Arithmetic operation between a 3D and a 2D files ADw Arithm 3D 2D ADHOCw AIRDE operation between G Je aad a EO te Input a file Fl Input 2D file F2 _ Choose file Output 30 file FS Choose file Anthmetic operation Value of An F3 4 F1 B F2 0 F3 4 F4 F2 6 F3 A F1 F2 B Value of E Set B to minimum null Use an execution mask Set E to masimur Value of C Store macro Set C to minimum nul file C ADHOCw HELP adwt1_B7 htm 1 of 4 15 02 02 09 34 40 ADwT1 mixed arithmetic operations Store macro Set Coto minimum nul Fe Execute Help Abort Set C to makimurn This programs allow to treat cubes with the information of images example flat fields The user has the following possibilities in which F1 is the input 3D file and F2 represents the 2D input file F3 is the 3D output file F3 F1 F2 A B F3 A F1 B F2 C F3 A F1 F2 B F3 A F1 F2 B The user must provide the names of the input and output files and the values of the floating variables A B and C It is possible to enforce the B or C values to minimum or null value 3 1E 38 or to maximum value 3 1E 38 If the result is less than 3 1E 388 the value is
176. HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located on the adhocw help adhocw htm file This file is adwt1_a3 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_a3 htm 2 of 2 15 02 02 09 34 21 ADw3D wavelength maps ADw3D Return to main ADHOCw help Return to main ADw3D help Getting wavelength maps The wavelength maps folder is enabled only if the phase map is loaded The display is similar to the interferograms folder display pute Becom Recompute computes the wavelength maps from the parabolic phase and the interferograms Actualize display displays the wavelength maps with the new display parameters Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_g htm file C ADHOCw HELP adw3d_g htm 1 of 2 15 02 02 09 34
177. IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_c htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_c htm 5 of 5 15 02 02 09 33 50 ADwT1 ADWT1_D full size part 1 i ADHOCw 2D display no ADC context 2D small area images Mono_ORG AD2 Export display to BMP Setup printer Print a Save ADC context Help XM Quit the programy 512 i 512 lz 11 Mouse arga 1 Cursor eee area 2 zoom 19x19 pix ai txt pix pix v Whole image image Parameters Image 20 files jh an ag Palette Threshold Step Levels overlap Color isophotes Nb max isoph File 01 5 quare pixels x R ainbow a 10 No H File 02 Phas_prb AD2 Isophotes 7 fo fi 0 0 White 7 399999 Change Suppress File 03 Chan Suppress File 04 Change Suppress File 05 Change Suppress File 06 Change Suppress P Mask file 1 with file 2 values gt 3D files File name Visible Color Drawing Cell size pixels Normalization Background First chnl Last chnl Chnil offset Intens offset File 11 Change Suppress File 12 a Chan nge Suppress File 13 us Suppress file C ADHOCw HELP adwedd1t htm 15 02 02 09 33 51 ADW2D ADW2D_D full size part 2 HADHOCw 2D display
178. ITS formats for display programs only Cigale This program manages access to network files on other computer disks Windows 32bits Select a page of menu About Help x Quit File Translator Possible normalization of conversions new_value 4 old_value B A 11 0 B 0 0 The ADHOCw File Translator allows to convert 2D and 3D files It reads and writes various data file C ADHOCw HELP adwft htm 1 of 3 15 02 02 09 34 05 ADwET File translator module formats ADHOC FITS IDL binary and others If you ignore the type of a file use the File_ parameters function to get the information 3D gt 3D converts a 3D files ordered by spectra or ordered by channels 2D gt 2D converts a 2D file 3D gt 2D slices converts a 3D into a set of 2D files 2D slices gt 3D converts a set of 2D files into a 3D file File_parameters gets the file type allows to modify its parameters and gets mini amp maxi data values Dump and modify give a direct reading and writing access to the data Macros are automatic batches to convert sequentially several files When you convert files you can adjust the conversion by using the A and B variables located in the left bottom part of the main window The translation is new_value A old_value B If the result exceed the dynamics of the output format values are set to the minimum or maximum possible values 2D or 3D simple translations 3D
179. ITSIO to correctly construct or to parse the keyword records rather than try to deal directly with the raw FITS formats file C ADHOCw HELP adw_what htm 13 of 15 15 02 02 09 33 45 ADw what is ADHOCw Each Header Unit begins with a series of required keywords which depend on the type of HDU These required keywords specify the size and format of the following Data Unit The header many contain other optional keywords to describe other aspects of the data such as the units or scaling values Other COMMENT or HISTORY keywords are also frequently added to further document the data file The optional Data Unit immediately follows the last 2880 byte block in the Header Unit Some HDUs do not have a Data Unit and only consist of the Header Unit If there is more than one HDU in the FITS file then the Header Unit of the next HDU immediately follows the last 2880 byte block of the previous Data Unit or Header Unit if there is no Data Unit 6 ADA and ADT photon counting formats The ADA format ADHOC Acquisition is connected the photon counting acquisition program ADwIPCS The format is binary There are 3 possible modes which are automatically recognized by the programs simple 256x256 coordinates 2 bytes long coordinates 4 bytes successively Y and X long coordinates and frame count 8 bytes successively X and Y 2 bytes each one The 4 remaining bytes is a 30 byte frame count long integer shifted of 2 bits on the le
180. LI DEF and C ADA DEF ASCII files during this step there is some danger if the light is in the dome Third stage is up to 10800V this value is defined in the GHASP DEF CHILI DEF and C ADA DEF ASCII files which is the maximum THT during this step the danger is maximum the intensification is high and the tube is in counting mode The user must check continuously the photon images on the TV control screen and decrease THT if necessary Permanent illumination of a pixel is strongly forbidden because it burns definitively the channeltron i e the pixel the tube will be quickly damaged When the THT is high the user can tune the voltage manually with a track bar If he clicks inside the white task bar the change is only 1V Dragging is also possible Down buttons are urgency buttons and their effect is immediate LE ADHOCw tuming THT Biel Es ADHOCw Photon Counting Up to 6000 W Down to 6000 Y Up to S400 w Down to 9400 V Up to maximum 10800 V Tune manually up to maximum Stop positionning Down to0 Y _ S400 y Track cursor to change THT Click inside the white trackbar to change only a step of 1 Volt 10800 we The shutter is directly managed from the acquisition window file C ADHOCw HELP adwi_c htm 2 of 3 15 02 02 09 34 02 ADwIPCS THT It can be opened or closed It can also be closed automatically if the photon rate exceeds a given value which is a strong protection to high accidental illumin
181. LP adwft_a3 htm 2 of 2 15 02 02 09 34 05 ADwT1 ADA IPCS integration ADwT1 Return to main ADHOCw help Return to main ADwT1 help E01 Integration of photon counting ADA files H Dw integration of ADA files ADHOCw Aegean of AGA OO COURTE Hes Input reference ADT file Choose file Hormalize exposure from frame count recommended M Correct from remanence recommended within same pixel Mote Hat after computation Me logbook informe of the stahstce of the number of remanent photons founded per pixel shitt Usually tame pixels adequate Remanence corection is nol suggested for calibrations saturation risk but is strongly recommended for the abject itself increase of S M M Suppress external TV parasites recommended aboye sigma 5 Integrate cycles from i to Output 36 DAS tile sum This function transforms a set of frame ADA photon counting files into an integrated AD3 file C ADHOCw HELP adwt1_e1 htm 1 of 5 15 02 02 09 34 06 ADwT1 ADA IPCS integration cube The program recognizes automatically the different ADA input files as indicated in the ADT log file 2 bytes 256x256 4 bytes or 4 bytes frame count Normalize exposure from frame count allows to ponderate the different ADA_ input files with the real photon counting rate If the CPU was abnormally busy during acquisition or if the counting rate was too high it is possible that some frames were not counted I
182. Lower 18 31 10 frame rejected 56 photons 0003 01 Lower 18 31 10 D M31_GHASP G016 G0160101 ADA frames rejected 1 remains without remanance 85 0 0003 01 Lower 18 31 11 moy sig discri 8 4 4 3 30 0003 01 Lower 18 31 11 D M31_GHASP G016 G0160201 ADA frames rejected 0 remains without remanance 81 8 0003 01 Lower 18 31 11 moy sig discri 8 4 4 5 31 0003 01 Lower 18 31 11 frame rejected 33 photons 0003 01 Lower 18 31 11 D M31_GHASP G016 G0160301 ADA frames K 0 ected 1 remains without remanance 81 8 8 31 31 moy sig discri 9 0 4 9 34 Lower 18 31 31 frame rejected 35 photons 8 31 31 frame rejected 43 photons 1 Lower 18 31 31 D M31_GHASP G016 G0160224 ADA frames cted 2 remains without remanance 83 2 3 01 Lower 18 31 31 moy sig discri 8 2 5 1 34 O O gt O HE K H He ODO D file C ADHOCw HELP adwt1_e1 htm 4 of 5 15 02 02 09 34 06 ADwT1 ADA IPCS integration D U FH SE OQ KH 0003 01 Lower 18 31 31 frame rejected 37 photons 0003 01 Lower 18 31 31 frame rejected 46 photons 0003 01 Lower 18 31 31 frame rejected 40 photons 0003 01 Lower 18 31 31 D M31_GHASP G016 G0160324 ADA frames ejected 3 remains without remanance 83 4 0003 01 Lower 18 31 31 Normalizing resulting file energy onservation 1 01
183. ML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_ba htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_ba htm 6 of 6 15 02 02 09 34 07 ADwET slices ADwFT Return to main ADHOCw help Return to main ADWFT help 3D slice translations To build a cube from a set of 2D images slices or to split a cube into a set of 2D images click on the 2D slices gt 3D or 3D gt 2D slices folders When you select the slices input files in the 2D slices gt 3D mode or when you select the slices output files in the 3D gt 2D slices mode the following screen will appear file C ADHOCw HELP adwft_a2 htm 1 of 4 15 02 02 09 34 07 ADwET slices Ex ADWFT Slices definition Definition of the input slices 1 2D slice of reference ou must first indicate the name of a 20 file which ts the 20 slice of reference and the tatal number of channels The reference is a slice file and can be the file name of one of the channels E WB x FORMAT SSCFHT 31 0922c fit Indicate reference Number of channels 27 lo ta nest stem 2 Slices masks ou must now define the slice mask The slice mask is similar to the reference slice name defined in 1 Channels number will be incremented inside the slices f
184. OCw help Return to main ADwT1 help Pytheas functions G How to reduce PYTHEAS AD aDwT1 sh152 a x Version Hide task manager window Bring task manager to front AD H OCw ADwT1 2001E JBx Obs Marseille 1280 x 1024 96 ppi General 2D 3D operations Cigale Profiles IPCS Tiger Pytheas miscen G01 PYTHEAS creation of the 3D wavelength cube EZ Display control Help Quit the program Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions For that press the Show logbook button above at any time file C ADHOCw HELP adwt1_g htm 1 of 2 15 02 02 09 34 57 ADwT1 menu PYTHEAS Jj G01 PYTHEAS creation of the 3D wavelength cube Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_g htm Return to main ADHOCw menu Retur
185. OCws_plus BLAISOUS Phas_prb AD2 Dutput not dephased 3D file Choose file Correct seeing and displacement C Correct seeing only Correct displacement only The correction will be done only for channels for which the seeing is less than the maximum seeing At default maximum seeing is put to the largest value of the seeing of the i channels f Use an execution mask fou can put it at any value scroll table to Pa Execute Help X Abort EX store macro Avoid interpolations win 50 excuting time S This function is used to correct CCD observations from the variations of the seeing WARNING the execution of this function is very long 1h30 with a Pentium 11 450 MHz for 512x512x27 45mn without interpolations The input ADS seeing parameter file is issued from ADHOCw functions C06 or C07 is ASCII and has a file C ADHOCw HELP adwt1_c8 htm 1 of 4 15 02 02 09 34 50 ADwT1 special ADS format When the ADS file name is given the program first scans the seeing values in order to indicate the channel with the worst seeing larger value and inserts this value in the Maximum seeing allowed box In principle all the channels must be corrected in order to fit with the worst seeing But if only 1 or 2 channels have an extremely bad seeing compare to the others the user can change the maximum seeing allowed value in order not to decrease too much the spatial resolution In this case all the
186. PHASE fin D ADHOCws_plus BLAISOUS Call1 da3 ph_bru D ADHOCws_plus BLAISOUS Phas_bru AD2 ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 cal_sum D ADHOCws_plus BLAISOUS Sum_cal AD2 cal_rv D ADHOCws_plus BLAISOUS RV_cal AD2 x11 6560 000000 xc 257 50 yc 262 50 ellipt 1 00 center 1 elliptCCD 1 p_pf 1162 Imbd_p 6562 780 Imbd_cal 6598 953 Imbd_scancal 6598 953 lmbd_obj 6562 780 Imbd_scanobj 6571 640 minangle 0 000 maxangle 360 000 minradius 0 000 maxradius 99999 000 algorithm 1 chg_chnls 2 keyword options PHASE pasi 3D n e file name with whole path calibration cube ph ph_bru 2D output 2D output file with whole path rough phase with whole 2D output file with whole path rough phase rough phase a prb 2D output file with whole path parabolic phase cal_sum 2D output file with whole path sum of the calibration channels cal_rv 2D output file with whole path radial velocity of the calibration through the parabolic phase xl1 wavelength reference of channel 1 lt _ sa XC OoOO approximate center of the rings X coordinate center approximate center of the rings X coordinate the rings X coordinate yc approximate center of the rings Y coordinate file C ADHOCw HELP adwt1_c1 htm 4 of 6 15 02 02 09 34 17 ADwT1 phase computation ellipt approximate ellipticity value X Y pixel ratio 0 check t
187. Prime matriz LF D L Ja D h 1 1 D LL Ja D h G Sapian puerta 3 i a a A a eT T j caisainn Fara 29007 LC EC CO CS P P O CT C Lorentzian FAHM 24001 Smaothing pla Sims i FO O OO e ao nA mo on PUR ao ON M L CO AGr SAINT sour anr uaia e tit file with user unkan wal hee TN nu vale 0 LR LE 0 D t LR D LE a b LE J D i Less anessin tt 2 Aure urarru MC ROUE O O O OO ROUEN OR OO On mn E of Ltecute Le Ip ji a LES z z a User tnmoothivs sar tek and sek cefved tmootbias nze a12 sc ua manie The program accepts 2D or 3D input files it recognizes automatically the type of the input file The smoothing pattern values are displayed on the right part of the window If the matrix is larger than 17x17 values only the central ones are displayed The user can choose different pre defined smoothings square gaussian lorentzian 5 pixels patters or give its own smoothing pattern from an ASCII user file At any moment the user can update the displayed values by pressing the Update matrix button and print the matrix by pressing the Print matrix button In addition an execution mask possibility is available Square mode it is a Dirac function with a width given in integer pixels file C ADHOCw HELP adwt1_b9 htm 2 of 6 15 02 02 09 34 42 ADwT1 spatial smoothing Gaussian mode is a gaussian cur
188. Quit the program 7 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions For the moment no function is implemented in this section file C ADHOCw HELP adwt1_d htm 1 of 2 15 02 02 09 34 55 ADwT1 menu PROFILES Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_d htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_d htm 2 of 2 15 02 02 09 34 55 ADwT1 menu IPCS ADwT1 Return to main ADHOCw help Return to main ADwT1 help IPCS photon counting observations functions E 2 ADw ADwT1 Biel E _Bringtask managertohent ADHOCw ADwT1 Version 1 00 JBx 1280 x 1024 96 ppi E01 Integration time normalization and remanence cleaning of ADA files Edit a batch file H Exec a batch file Quit
189. Type of source t 2D image TINTIN TENTE ENTER 3D calibration Silevsasebenensest deveesen tbabdedsendedsodvscauntsedea 3D object Random nbptsframe pm ADHOCw Scanning parameters 3D calib F 6598 953 6562 780 IV see saw scanning recommended 3B object Current 4 Ait AL 6562 780 9 210000 Perot Fabry scanning mode Scanning performed Scanning HOT performed Scanning with PAUSE before channels nb of channels exposure time per channel seconds maximum number of cycles scanning wavelength A starting channel number starting cycle number Queensgate constant Scanning controler CS100 interface Parallel Chili Serial RS232 GHASP C Test file Disk storage Change Directory de ET ae E Data format li x and Y 256 x 256 2 bytes Data file names Miiicckk ADA short file name Photon data files from G1240101 A4DA to G1249924 ADA Observation log file G124 ADT file C ADHOCw HELP adwi_it htm 15 02 02 09 34 01 Matrox board error control normal MIL errors recommended C full MIL errors tests only X Quit Tests Matrox PF eh Print this window Remote Controls permanently updated Base default instrument parameters PRECEDENT VALUES Shutter UNDEFND Open Close THT sent EEE Tune THT read 3999904 CloseLoop NOK Inhib closeloo
190. Y Z translation for 2D or 3D files B12 Sort eliminate interpolate profiles on sigma for 3D files ex cosmics B13 Suppression of continuum at pixel level for a 3D file Quit the program B14 Correction of wrong lines columns or channels of a 2D or 3D file B15 Photometric correction channel channel from ADX file 9 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions file C ADHOCw HELP adwt1_b htm 1 of 3 15 02 02 09 34 36 ADwT1 menu OPERATIONS 2D 3D B01 Total sum 3D gt 2D B02 Extract a 2D channel from a 3D file BO3 Insert a 2D channel into a 3D file B04 Get minimum and maximum of a 2D or 3D file B05 Arithmetic operations on a 2D or 3D file Fout f F1 B06 Arithmetic and masking operations between 2D or 3D files Fout f F1 F2 B07 Arithmetic operations between a 3D file and a 2D file Fout3D f F3D F2D B08 Spectral smoothing on a 3D file B09 Spatial smoothing on a 2D or 3D file B10 Extraction of a sub cube 3D or a sub image 2D B11 Rotation scaling XYZ translation and inversion for 2D or 3D files B12 Sort eliminate interpolate profiles on sigma for 3D files ex cosmics B13 Suppression of continuum at
191. Y correction 0 000 kms y Save on ADP file 7 Help x Abort don t save Identification is a free ASCII text written by the user to recognize his observation Dimension of the cubes have no limitations Z is usually the lambda dimension which is often the number of channels Extraction corner is a user information which keeps track of a possible further extraction from a larger cube all positions are numbered from 1 file C ADHOCw HELP adwt1_ad htm 2 of 5 15 02 02 09 34 20 ADwT1 ADP parameter files Spectral information allows 2 modes the Perot Fabry mode and the Spectrography mode In the Perot Fabry mode you give the interference order of the interferometer relative to a given wavelength which is completely disconnected from the line wavelengths or the scanning wavelengths You must also give the line and scanning wavelengths for both calibration and object When the user press the button Update values the interfringe values in Angstroems and in km s are automatically computed The wavelength of channel 1 is the reference wavelength for the de phased cubes This last parameter can be changed until the phase map computation In the Spectrography mode the only useful parameters which must be given by the user are the length of the spectrum in Angstroems and the wavelength of the first spectral element When the user press on the button Update values the length of the spectrum in km s is compute
192. YTHEAS CUBE Info Reference origin position in output frame 25 12 0182 16 Batch Lower 18 16 22 G01 PYTHEAS CUBE Info Step 1 computing file C ADHOCw HELP adwtt_g1 htm 6 of 14 15 02 02 09 34 36 ADwT1 PYTHEAS 1 reference channels and exact etalon interference order 0182 16 Batch Lower 18 16 22 G01 step 10 0182 16 Batch Lower 18 16 22 G01 step 10 0182 16 Batch Lower 18 16 23 G01 547 step 10 0182 16 Batch Lower 18 16 23 G01 547 step 10 0182 16 Batch Lower 18 16 24 G01 547 step 10 0182 16 Batch Lower 18 16 24 G01 547 step 10 0182 16 Batch Lower 18 16 25 G01 547 step 10 0182 16 Batch Lower 18 16 25 G01 547 step 10 0182 16 Batch Lower 18 16 26 G01 547 step 10 0182 16 Batch Lower 18 16 26 G01 547 step 10 0182 16 Batch Lower 18 16 27 G01 547 step 10 0134 16 Batch Lower 18 16 28 G01 intense calibration line 1 0182 16 Batch Lower 18 16 28 G01 channel 25 874 0 873 0182 16 Batch Lower 18 16 28 G01 channel 24 488 0 534 0182 16 Batch Lower 18 16 28 G01 orders within a range of 5 from origin 0182 16 Batch Lower 18 16 28 G01 7 295 channels 0182 16 Batch Lower 18 16 28 G01 6 971 channels 0182 16 Batch Lower 18 16 28 G01 6 647 channels 0182 16 Batch Lower 18 16 28 G01 6 324 channels 0182 16 Batch Lower 18 16 28 G01 6 000 channels 0182 16 Batch Lower 18 16 28 G01 5 676 channels PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_
193. a 6562 78 Ly alpha 1215 67 H b ta 4861 32 H gamma 4340 46 H delta 4101 73 Hepsi 3970 07 NII 6583 37 NII 6548 06 NII 6527 4 NII 5754 57 OIII 5006 86 i OIII 4958 93 i OIII 4931 0 i OIII 4363 19 i OII 3726 04 OII 3728 80 OII 7330 19 OII 7319 92 i SII 6716 4 SII 6730 8 m v Cahbraton wavelenth s 4537 754 4704 395 4708 862 Ne I 4710 067 4712 066 4715 346 4788 927 4827 344 4884 917 4957 033 5330 777 5341 094 5343 284 5400 562 5764 419 5852 488 5881 895 5975 534 6029 997 6074 338 6143 062 6163 594 6217 281 6266 495 H lium 3888 648 4471 479 5015 678 He I 5875 691 5875 966 6678 151 7065 190 10829 088 10830 248 10830 337 17002 38 18685 96 18696 94 i file C ADHOCw HELP adwt1h10 htm 1 of 3 15 02 02 09 35 04 ADwT1 Common wavelengths Nebular wavelengths H alpha 6562 78 A Ly alpha 1215 67 A H b ta 4861 32 A H gamma 4340 46 A H delta 4101 73 A H epsi 3970 07 A NII 6583 37 A NII 6548 06 A NII 6527 4 A NII 5754 57 A OIII 5006 86 OIII 4958 93 OIII 4931 0 OIII 4363 19 OII 3726 04 OII 3728 80 OII 7330 19 OII 7319 92 SII 6716 4 SII 6730 8 OI 6363 82 OI 6300 31 OI 5577 35 Calibration wavelengths N on 4537 754 4704 395 4708 862 Ne I 4710 067
194. a htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_ma htm 3 of 3 15 02 02 09 34 16 ADw3D loading phase ADw3D Return to main ADHOCw help Return to main ADw3D help Loading the phase The phase is necessary to compute the wavelength maps from interferograms and to get the rough monochromatic continuum and velocities maps specially during observations The request phase is the parabolic phase for instance PHAS PRB AD2 file which is obtained from the ADwT1 program function C01 The operation which loads the 2D parabolic phase is available in the Phase folder where the phase map can also be displayed the overlap checkbox is automatically checked in order to display clearly the different interference orders but uncheking this box will display really the parabolic phase map file C ADHOCw HELP adw3d_f htm 1 of 3 15 02 02 09 34 16 ADw3D loading phase Input format of the parabolic phase map AD2 file Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_f htm fil
195. ade crowns Ix 1256 ly 1256 lz 11 Ex Export display to BMP j By Setup printer m BP Print i Save ADC context 7 2 x Quit the progran se xt pix 1 xt pix Mouse arga Mouse arga 2 zoom 19x19 pix v ha Whole image Parameters Image Mini 2149 Display parameters Flip vertivally Graph ares Visualization mode Square pixels file C ADHOCw HELP adw2d_k2 htm 6 of 12 15 02 02 09 34 27 Maxi 2451 Flip horizontally alett Rainbow X Scale max 2420 Threshold 2100 0 1 01 1 10 10 100 100 40 10 300 100 SS 000 1000 Scale min 2100 Scale overlap Actualize full display More zoom Action of the left button of the mouse C Cross sections Integration of profile C Image modification C Text overlay Kinematics of galaxies e aen of eyes Fareme tae Danse a k ET TIS Selector Load file Save to file M automatic saving AAAA Par TIENESS Projected rotation C Fixed parameters Params fr Edit a params r array amp raph PAIRE fers ENEJ all 4 quadrants EJES CROWNS blue red crowns 4 pix 128 0 2120 0 km s Rmin pix Vin Rmarj128 0 pik Wmax 2 f Redraw graph ADw2D kinematical functions user made crowns l l VIMS BUI IY PORS All the display functions rotational velocities mouse movement consider the
196. adial velocities values per channel This function gives the correspondence between the channels and the wavelength or the radial velocity with heliocentric correction H ADWT1 A02 Informaation on channels 02 20 02 1999 22 35 43 a dag 1162 at 6562 78 Angstroens 6598 95 Angstroers 6598 95 Angstroers 6562 78 Angstroens 6571 64 Angstroens D kna s 0 ka s Object lambda at rean RY 62 78 Angstroers 0 00 kn s Interfringe S i E Angstroers Interfringe f 92 kn s One channel 0 2 Angstroers One channel 9 55 kna s Reference dephased channel 1 6571 64 Angstroens 1 Channels gt wavelength Angstroems Chnl 3 2 1 0 1 2 3 6543 06 6548 71 6554 35 6560 00 6565 65 6571 29 6576 94 6543 27 6548 92 6554 56 560 6565 85 6571 50 6577 15 6543 48 6549 13 6554 77 6560 4 6566 06 6571 71 6577 35 6543 69 6549 34 6554 98 0 63 6566 27 6571 92 6577 56 6543 90 6555 19 60 6566 48 6572 13 6577 77 6544 11 349 7 6555 40 S 6566 69 6572 3 6577 98 6544 32 6555 61 1 6566 90 6572 5 6578 19 rm mm me INI ON UT me ON b The interfringe modulo is computed for i 3 to i 8 This is an example of the printed or saved text ADHOCw ADwT1 Information on channels A02 20 02 1999 22 18 34 Parameter file Blaisous adp Nb of channels 27 Interference order 1162 at 6562 78 Angstroems Calibration reference lambda 6598 95 Angstroems Calibration scanning lambda 6598 95 Angstroems Object zero
197. ages The Parameters folder allows to define up to 6 image files For all of these images you can give all the visualization parameters These images can be superimposed or blinked The default mode is superimposition of all the images The first file is first displayed then the second aso Pixel modes square or smoothed overwrite the image area while isophotes are superposed When the Image folder is selected the composite image is displayed A text label indicated what is the pixel type image which is seen The step threshed scale and other parameters refer to this image and if you change them only the display parameters of this file will be changed The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page file C ADHOCw HELP adwa2d_c htm 1 of 5 15 02 02 09 33 50 ADw2D mixing different displays of images LS ALUHO Cm ZU desplurs ou ADC contest 52 i ii Tad h fae MAC Le l Er k big al kids RR ihn ht c a Dissspcerit Putt X Lane sexe va Mouceaise Case Hoe yes fm tt rl fic pe Ph rage nerd nya A les ASTE CETE TE DETE d Faits Lkr g Shoo ath oc aE Loki aghdes Mb agh 7 1 Sis 134 se wes arcs T f 0 iHe gi Crasas geaca Mapa iep veces je roc wis Pex Crags Tgp 7517 G
198. al process or users and can be located on other computers accessible on the network Macro definition Example ARITHM fin D ADHOCws_plus BLAISOUS Call da3 fout D ADHOCws_plus BLAISOUS bidon ad3 oper 0 a 1 000000 b 0 000000 file C ADHOCw HELP adwt1_b5 htm 2 of 4 15 02 02 09 34 39 ADwT1 arithmetic operations keyword content options ARITHM 2D or 3D input file name with whole fin path 2D or 3D output file name with whole fout path oper type of the arithmetic operation 0 gt F2 A F1 B 1 gt F2 alog10 F1 A B 2 gt F2 In F1 A B 3 gt F2 10 F1 A B 4 gt F2 exp F1 A B 5 gt F2 A 6 gt F2 sqrt F1 A B 7 gt F2 F1 A 2 B a floating variable used in the operation b floating variable used in the operation Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0232 01 Lower 11 52 08 Files are 3D Fl input F2 output 0232 01 Lower 11 52 08 Operation F2 A Fl B 0232 01 Lower 11 52 08 with a 1 000000 and b 0 000000 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser file C ADHOCw HELP adwt1_b5 htm 3 of 4 15 02 02 09 34 39 ADwT1 arithmetic operations incorporated to ADHOC But the ADHOC
199. ame rejected 56 photons 0003 01 Lower 18 31 10 D M31_GHASP G016 G0160101 ADA frames rejected 1 remains without remanence 85 0 Moy is the mean number of photons per frame in the ADA file Sig is the sigma of photons per frame Discri is the maximum accepted Frame rejected indicates individually the number of photons of the rejected frames file C ADHOCw HELP adwt1_e1 htm 2 of 5 15 02 02 09 34 06 ADwT1 ADA IPCS integration The for every file the total number of rejected frames and the final count in without remanence is written At the end the final statistics are given 0003 01 Lower 18 31 31 Normalizing resulting file energy conservation LOL 0003 01 Lower 18 31 31 Writing result 0003 01 Lower 18 31 42 Global statistics on photons 0003 01 Lower 18 31 42 Nb photons of remanence with 0 pixel shift 40145 16 5 0003 01 Lower 18 31 42 Nb photons read 244011 remnants 40145 final 195406 80 1 The input file are IPCS files ADA ADT The output file is created as new ADHOCw type AD3 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example INTEGR_ADA fin D M31_GHASP G01
200. and F02 This function creates a new cube in a new directory with new dimensions Procedure 1 the program computes the exact interference order and the zero wavelength of the first calibration line For that it looks to every lens and computes coincidences between calibration lines Only the range within 5 around the reference interference order is computes 2 then the program bufferizes the 3D individual object spectra 3 and builds the output 3D file following the output geometrical sampling For every output pixel the program finds the 3 nearest micro lenses and computes the final spectrum In order to set correctly the zero wavelength the program takes in account the exact position of the calibrations lines and spots for every micro lens The result is in a different directory because 3D dimensions are different from the input To check before execution tuning of the etalon Use ADw3D on the calibration file and see on different channels if the spots appears simultaneously This effect is corrected by G01 but it is better to know its importance file C ADHOCw HELP adwt1_g1 htm 1 of 14 15 02 02 09 34 35 ADwT1 PYTHEAS 1 To check after execution computed exact order log information nb of total measured spectra log information set as input a copy of the calibration file and check the result This gives insurance that the zero wavelengths and dispersions are correctly computed for every indivi
201. annel 1 as default Starting cycle number the observer can decide not to begin at cycle 1 as default Calibration scanning wavelength For instance 6598 953 A Object scanning wavelength For instance 6562 78 A Queensgate constant is different for each controller and each Perot Fabry interferometer See saw scanning organizes the scanning in order to scan in increasing mode the odd cycles scans and in decreasing mode the even cycles If this box is not checked all the cycles are scanned in increasing mode See saw mode decreases the effects of transparency and seeing variations over the observation This mode is recommended The ADw3D program manages the waiting of the channels in every case How to switch quickly from calibration to object parameters or the inverse first edit correctly the default values under the 3 columns named 2D 3D calib and 3D object in the Scanning parameters box These new values are now default values and will be automatically stored in a system file in order to keep this information file C ADHOCw HELP adwi_a htm 2 of 7 15 02 02 09 34 00 ADwIPCS Parameters second simply click on the correct mode in the Type of acquisition box the current values will immediately change if you wish to change at this moment some current values you can they will be also kept on the system file until you click again in the Type of acquisition box Perot Fabry sc
202. anning mode Scanning can be performed or not interferometer is controlled or not If the scanning is requested with pause the program stops and requests an action of the user before each channel acquisition It is very useful for tuning an instrument for example to tune focus simply create as many images as channels Scanning controller CS100 interface Two different interfaces exist on the CS100 controllers of Marseille s Observatory Parallel is used in Chile or at Byurakan Serial is used at Marseille OHP 6m The serial port can be COM1 COM2 COM3 or COM4 Disk storage The directory is the directory where the data and log files will be written The dialog allows to create directories The data format can be of two kinds only 4 bytes per photon X and Y coordinated in a 512x512 frame This is the default 8 bytes XY coordinates frame number useful for time resolution applications The data file name code can be of 2 kinds Pooocckk ADA short name usually used Pooooooocccckkkk ADA exceptional long name where P prefix 1 character o00 number of the observation 3 or 7 characters cc number of the cycle kk number of the channel If the observation number must be more than 999 or the cycle number more than 99 or the channel number more than 99 the second format must be used The file log will be Pooo ADT or Pooooooo ADT Matrox board error control When acquiring in normal mode there
203. as new ADHOCw type AD3 file C ADHOCw HELP adwt1_c2 htm 1 of 3 15 02 02 09 34 51 AdwT1 wavelength computation This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example LAMBDA fin D ADHOCws_plus BLAISOUS Call1 da3 ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 fout D ADHOCws_plus BLAISOUS call_p ad3 keyword content options LAMBDA fin 3D input file name with whole path phased cube ph_prb 2D input file name with whole path parabolic phase fout 3D output file name with whole path dephased cube Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present file C ADHOCw HELP adwt1_c2 htm 2 of 3 15 02 02 09 34 51 AdwT1 wavelength computation HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file
204. asons Computer information Computer Time Universal Time jo hours m Clocks H M 5 H M 9 H M 5 ComputerTime Universal Time Sideral Time 15102001 foo foo joo lt adjust computer clock X Quit Help file C ADHOCw HELP adwt1_h7 htm 1 of 3 15 02 02 09 35 01 ADwTI sideral clock 18 10 2001 fo foo foo ee adjust computer clock This program displays a real sideral time clock Site information choose the observatory site Computer information indicate the difference between the internal computer clock and the Universal Time Adjust computer clock preselect the values and press the button Adjust computer clock at the second in order to set the internal computer clock Log book results None Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h7 htm file C ADHOCw HELP adwt1_h7 htm 2 of 3 15 02 02 09 35 01 ADwT 1 sideral clock Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_h7 htm 3 of 3 15 02 02 09 35 01 ADwT1 Interference filters ADwT1
205. at the pointed channel the current wavelength and the current radial velocity are displayed in real time when the mouse is moved The direct and barycenter modes are similar of the ones in the mail window To select Zoom there are 2 ways select an area to enlarge with the mouse or type directly the coordinates X and Y in the upper editable positions To select an area to enlarge with the mouse click and drag with the mouse right button and click on the Zoom area button above the graph to execute zoom To select an area to enlarge with the keyboard type X and Y rectangle values in the corresponding boxes and click on the Zoom area button above the graph to execute zoom An example is shown below file C ADHOCw HELP adw2d_zp htm 2 of 7 15 02 02 09 33 56 ADw2D zoom on profiles ADw2D integrated profile X Return to main window __Zoomares from 4006505 to 980 8841 Oo vaos vac DEEE Pv EERE No smoothing z Full spectum from 6520 000 to 6610 000 Direct Bilis Bayoenter chi MEMME Limb KG left mouse button Free graph Tabel for the user in order to identify or date graphs printir J This label can be edited To zoom define a rectangle by pressing the 880 8841 6520 000 6610 000 400 6505 LE AMCRA mye file CI ADHOCW HELP adw2d_zp htm 3 of 7 15 02 02 09 33 56 ADw2D zoom on profiles Enlarged graph ADw2D integrated profile Re Eull spectrum Xirom en fen 231 to 5570 807 Di
206. ated 0248 Phase computation T 00 01 04 02 0249 Wavelength maps 00 00 1 0250 Dummy operation 00 00 00 00 00 00 00 00 16 00 00 00 ADHOCw task manager 00 01 04 00 00 00 EE 00 00 00 EME suspend RES Suspend Res Suspend Res ous Hic ne AUOT Abort gt Abort ne ADOT AUOT Aborn AHOT gt ADOT BDOTI AUOT ADOTT 00 00 00 Abort 00 00 00 EME 00 00 00 Sus Task JE reserved to macro batchs 16 terminated 0247 M Bring general menu to front 00 0 00 00 35 When you run a function a task number is immediately allocated and every second a timer displays the percentage done the elapsed time the remaining time and the estimated time When the program is running you can suspend it by clicking on the Suspend button Then you can resume it by clicking on the Resume button abort it by clicking on the Abort button change its priority by clicking on the or buttons If the priority becomes high or critical the system could have problems to answer to other requests as launching other programs or even control the task manager look to informations by clicking on the Infos button In this case the following window will appear file C ADHOCw HELP adwt1_ta htm 1 of 2 15 02 02 09 33 45 ADwT1_task ADw task info AMBDA fin D ADHOCws_plus BLAISOUS Cal1 da3 ph_prb D ADHOCws_plus BLAISOUS Phas_
207. ations ADHOCw photon counting Version 1 00 JBx i nn Cycles and channels Acquisition THT intensifier channel exposure 00000 per 0015s Start 10467 volts current channel 0000 0024 current cycle 0000 0099 BUSPpENG scanning wavelength 6562 780 Queensgate constant 2 3350 X Emergency THT stop Photon counting status standby object Cumulated Request deferred stop Instantaneous exposure time 00 00 00 System priorities photons s 842 total nb photons 000000000000 High frames s 25 written on disk 0000000 0 Mb Critic count efficiency100 total counting efficiency 0 A automatic from photon rate maxphis WUT VA this window ne in front TY parameters BB allow modification Dis Black lul of the TV parameters t jE def 51 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwi_c htm Return to main ADHOCw menu Return to main ADwIPCS menu file C ADHOCw HELP adwi_c htm 3 of 3 15 02 02 09 34 02 ADwIPCS acquisition ADwIPCS Return to main ADHOCw help Return to main ADWIPCS help During a
208. be 7 able 3 0 a Adobe Photoshop Image a Advanced Streaming Format File Bi Advanced Streaming Redirector File gt wees Details sur le type de fichier Ad Extension AD Type de contenu MIME AT On SOLVE avec ADW ap APpIgAE Click on Nouveau Type New type file C ADHOCw HELP adw_ass htm 2 of 6 15 02 02 09 35 05 ADw2D 2D display module Modification d un type de fichier Description du type AD HOC 2D image Type de contenu MIME r Extension par d faut pour type de conten T Actions Mouveau Modifier Supprimer Valeur par d faut M Confirmer l ouverture apres le t l chargement HR Annuler The Nouveau New add open and click on Modifier Modify D Permettre l aper u rapide M Toujours afficher l extension Op ration de modification pour le type ADHOC 2 ee Tr Annuler Application utilis s pour effectuer l action DADO Cw Adwed exe 21 Parcourir F Utiliser DDE The application for the specified action must be the program location and name and 1 which means to specify the name of the file to display file C ADHOCw HELP adw_ass htm 3 of 6 15 02 02 09 35 05 ADw2D 2D display module ADC extension Modification d un type de fichier Description du type ADHOC 2D contexte Type de contenu MIME Extension par d faut pour type de contenu T
209. be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output file is created as new ADHOCw type AD2 DA3 file C ADHOCw HELP adwt1_b6 htm 2 of 5 15 02 02 09 34 39 ADwT1 masking operations This function can use an execution mask When the execution mask doesn t allow the operation the cube value F3 is set to value of F1 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example ARITHM2 finl D ADHOCws_plus BLAISOUS Call da3 fin2 D ADHOCws_plus BLAISOUS call_p ad3 fout D ADHOCws_plus BLAISOUS bidon ad3 oper 0 a 1 000000 b 0 000000 c 0 000000 keyword content options ARITHM inie 2D or 3D input file name F1 7 with whole path find 2D or 3D input file name F2 7 with whole path fie 2D or 3D output file name F3 7 with whole path file C ADHOCw HELP adwt1_b6 htm 3 of 5 15 02 02 09 34 39 ADwT1 masking operations 0 gt F3 A F1 B F2 C oper type of the arithmetic operation 1 gt F3 A F1 F2 B 2 gt F3 A F1 F2 B 3 gt F3 maximum of F1 and F2 4 gt F3 minimum of F1 and F2 null not taken 5 gt F3 null if F2 is null value F1 else 6 gt F3 null if F2 is null value F2 else 7 gt F3 F1 if F2 is inside
210. c6 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_c 6 htm 7 of 7 15 02 02 09 34 48 ADwT1 mixing ADS seeing files Return to main ADHOCw help Return to main ADwT1 help ADwT1 C07 Merging several ADS seeing files ADw mix ADX ADHOCw Mergig of several AOS seeng paraneiers Hes Fill up to 8 input ADX file name boxes Input ADS lile H Input ADS tile Hz Suppress Input ADS lile 3 Suppress Input ADS file 4 Input ADS file HS Suppress pul ES ee Input ADS file 7 Input ADS file 8 Fill the output file names boxes Output ADS ASCII seeing parameters file file C ADHOCw HELP adwt1_c7 htm 1 of 5 15 02 02 09 34 50 Suppress Choose file SUPOTESS SUPRTESS Suppress Suppress Te Store macro ay PP ee ADwT1 mixing ADS seeing files nns uae SE ae Ld denis rc Le at math a Output ADS AS Ell seeing parameters file Output control BMP tile name EADH CwS_ plus BL AISOUS Seeing BMP This function is supposed to mix several ADS seeing files obtained from the ADHOCw function C06 with different weights The output result is an ADS file and is normalized This function is useful to mix the seeing result obtained from different stars in the same field Important note displacements are normally computed but for seeing the seeing obtained from different stars can be largely different T
211. cause is could be edited manually to suppress spectra for instance between the execution of the F01 and F02 functions The structure of this editable TXT file is simple one line per spectrum 4 integer coordinates ix1 iy1 ix2 iy2 Example 220 3 276 7 337 3 394 7 457 3 514 7 346 507 397 511 586 DOT 638 SLL 712 507 743 511 Example of superimposition of selection and spectra shape is represented with a high value 1E16 file C ADHOCw HELP adwt1_f1 htm 4 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 1 Extraction parameters Input 2D continuum file Choose file Output 2D verification spectra file extraction only Choose file D Pytheas SH1 52 TIGER_extracted AD2 2D input file intensity threshold to separate the spectra Maximum spectrum length in pixels Maximum spectrum width in pixels Minimum spectrum length for elimination in pixels Minimum spectrum width for elimination in pixels Geometric parameters 2 Geometric parameters from lens array This OPTIONAL STEP ahows fo ehmirete spectre which reference E appear oidss e of fhe micro fenses postions nn nh eh Nc a St are Peon kore eB es 2 ens M Eliminate spectra on position coherence R Lens array type hexagonal central position of the reference spectrum floating pix Y central position of the reference spectrum floating pix D1 delta X along resulting horizontal floating pixels a DY1 delta along resulting horizonta
212. ccessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_ta htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_ta htm 2 of 2 15 02 02 09 33 45 ADwT 1 data processing module ADwTt ADHOCw program for data processing Return to main ADHOCw help Generalities ADP parameter files Function menu window Task manager window Display control window Executing mask Batches Creation of files of different dimensions Null values Shared files and network access ADHOCw data files Global batch macro command procedure Menu A General Menu B 2D 3D operations Menu C Cigale Menu D Profiles Menu E IPCS Menu F Tiger Menu G Pytheas Menu H Miscellaneous This program requests a minimum screen of 800x600 with 16 colors and 96 pixels per inch If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode file C ADHOCw HELP adwt1 htm 1 of 2 15 02 02 09 33 46 ADwT1 data processing module Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC B
213. cessary the adquate values File name D ADHOCws_plus B LAISOUS bidon ad3 Identification Nb of dimensions 3 Scale pix fi 000000 Dimension X 512 Top left comer fi Dimension Y 512 Bottom right corner fi Dimension Z 27 Zoom fi 000000 Comment KK 2 dimension parameters modevis nbiso Threshold Palette Step 3 dimensions parameters Lambda 1st channel 6560 000000 Interfringe 5 643047 RY of 1st channel kms 0 000000 Interfringe kms 257 812439 Observed lambda 0 6562 779785 PF naden ca order fi 162 000000 Mean RY of the object 0 000000 Ref lambda for PF order 6562 779785 Heliocentric corr kms fo 000000 Save new parameters New file request Update You can edit the parameters of ADHOC 2D or 3D files and change them Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended file C ADHOCw HELP adwft_b htm 5 of 6 15 02 02 09 34 08 ADwFT files structure operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_b htm Return to main ADHOCw menu Return to main ADWFT menu file C ADHOCw HELP adwft_b htm 6 of 6 15 02 02 09 34 08 ADwFT
214. cessive channels indicates the number of successive file C ADHOCw HELP adwt1_c3 htm 1 of 4 15 02 02 09 34 52 ADwT1 monochromatic continuum RV maps increasing channels in the case of emission or decreasing channels in the case of absorption which determines the edge of the profile The method is the following beginning from the maximum of the line the program looks on both left and right channels until he finds nb of successive channels which inverse the sense of the profile Default value for the parameter is 2 1 is better for not noisy profiles 3 could be preferred for very noisy profiles if the number of channels is sufficient fixed levels the parameter Mono channels indicates a way to measure the base of the profile If this value is for instance 20 this means that this base is defined by the value of the channel for which 20 of the channels are more intense in the case of emission and 80 are less intense In this case the simple barycenter of the line is computed above this level Slope change is the default method The continuum computation can be done with 3 methods mean of the 3 lowest channels if in emission and mean of the 3 brightest channels if in absorption is the default value from intensity histogram is a method is a similar computation as the fixed levels above If the value is 10 this means that 10 of the channels are lower that the continuum and 90 of the channels are ab
215. cities from the calibration is a test The values of this file must be near zero Nevertheless if the calibration scanning wavelength of very far from the object scanning wavelength more than 30 Angstroems some residual rings can appear they correspond to the part of the spectrum which is not scanned Usually this small effect less than 2 km s has a parabolic shape if you draw a cross section through the image Note the cross section through this file could show 2 effects systemic deviation from zero could be due to a large difference of wavelength and or scanning beween calibration and object In this case as the thickness of the coating layers of the interferometer vary with the wavelength this could explain a global deviation up to 20 or 30 km s parabolic cross section the program corrects the phase for the object wavelength In this sense it computes what would be the exact channels if the phase was scanned at the object wavelength When looking to the calibration this gives a parabolic effect which is not an error The output information Max corr2 in the log file gives the maximum correction i e the maximum amplitude of the parabola The scanning parameters are important the interference order of the interferometer at a given wavelength is a data which is connected to the interferometer itself and is not affected by the observation parameters the calibration line is the spectral line which was obtained from
216. clicking left button of the mouse Define profile zones cr e Load 11 zones from ADZ file Close 11 zones mode SumMini SumMasi Profile displayed in zoom or image None v Superimposition of profiles Square in pixels Normalization individual S Draw profiles Continuum normal X Display parameters Graph area Image area te Rainbow Scale max 3360 Threshold 0 1 1 10 10 100 100 000 1000 Step 210 q 1 10 10 100 100 000 1000 Scale min 0 M Scale overlap Actualize display file C ADHOCw HELP adw3d_et htm 1 of 2 15 02 02 09 34 14 ADw3D full size ADw3D_E file C ADHOCw HELP adw3d_et htm 2 of 2 15 02 02 09 34 14 ADwT1 OH and or continuum substraction Return to main ADHOCw help Return to main ADwT1 help ADwT1 C04 Substract OH and or continuum from given areas This programs allows to substract parasite lines night sky OH lines for instance from the profiles AD Ti ADw OH suppression OI x ADHOCw OF and or continuum substaction Fam giver areas Input 3D file Choose file Recurrent substraction Wbx_portableMADHOCWs_plus BLAISOUSImbd_brut ad3 Input 80Z zones ASCII file Choose file WJbx_portable D ADHOCWS _plus BLAISOUS Zones _oh adz Output 3D file Jbx_portable D ADHOCWS _plus BLAISOUS Imbd_org AD3 Output control BMP file Choose file Jbx_portable D ADHOCWS_plus BLAISOUS 0H BMP Out
217. cquisition the green acquisition window is superimposed on the upper right part of the window Note that the two programs are completely independent ADwIPCS acquires the photons and writes onto disk ADw3D displays the arriving channels images ADw3D can be closed run again run simultaneously several times on different data When ADw3D is run again it can reintegrate easily the current observation IHI noirin 10467 suv uit CALIIL IE warg alala f FAST vasak liy objece L TPORTET EI coil Slrallur TT icine viant ETGT pm Y eeeamonte frre phinn rrin Aiutare L LEE LEE LUE LUE UE 1 mul che LULLUIL LUI 11 ted cuusiteny liceciny Ne win War po tach CE Atilt RE nwu we si a th a file C ADHOCw HELP adwi_d htm 1 of 4 15 02 02 09 34 03 ADwIPCS acquisition The acquisition window is the following The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page ADHOC IC 1A Y ph oton counting Vers Or 1 00 JBx Cycles and channels Acquisition THT intensifier channel exposure 00000 s per 0015s Start 10467 volts current channel 0000 0024 current cycle 0000 0099 peat NE scanning wavelength 6562 780 A Queensgate constant 2 3350 Photon counting status standby object Shutter Instantaneous exposure time 00 00 00 System
218. ction Return to main ADHOCw help Return to main ADWT1 menu A03 Heliocentric RV and precessions This function allows to compute heliocentric velocity correction and also precessions always useful l ADw Heliocentric RY Iof xi ADHOCw Hehocernttic RY and precession COMpUEUORS Coordinates of the object Alphad p fso hours fao minutes 50 67 Deitat F fs degrees 16 minutes 28 Epoch year 11950 seconds seconds Date of the observation Month Year Hour Minute Warning hours must be in Universal Time UT Compute heliocentric RV correction X Quit Results for the date of the observation Epoch 1997 48 apht f 6 r 22 mnfsss s Julian day 245062775 petat 45 deg t9 400 Computed value for heliocentric correction 3 14 km s This value is to add to all the measurements Current value stored file C ADHOCw HELP adwt1_a3 htm 1 of 2 15 02 02 09 34 21 The heliocentric correction will be automatically added to measurements The user must then copy the computed value in the parameters ADP file If he forgets the following message appears E ADw warning EX ADHOCw warning You didn t save the computed heliocentric correction in the parameters ADP file 2 Return to dialog to save heliocentric correction DR D MS DONS Nr RIT RANON j Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in
219. ction channel channel from seeing ADS file ei Show logbook Compute the calibration Finesse T Build custom made lambda cubes fot Display control Get photometric parameters from rough analysis of non dephased channels Continuum substraction from given areas Execute a function Quit the program 7 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions For that press the Show logbook button above at any time file C ADHOCw HELP adwt1_fc htm 1 of 3 15 02 02 09 34 29 ADwT1 function menu window Three areas can be distinguished on the ADHOCw ADwT1 window The menu inside several folders General Miscellaneous give access to the different functions Just double clock on the chosen function to run it The right area with 6 important buttons Execute a function executes the highlighted function which is similar to the double click mentioned above Display control which allows to access to graphics generated by the program For this look to the section Display control Quit the program or Help are easy to understand and to use Edit a batch file and execute a batch file allow to access to batch programming witch is the possibilit
220. ction procedures coloured paper if possible adwft_a3 htm adw_proc htm gt page 5 of adhocman doc 3 Program ADwFT coloured paper if possible adwft htm adwft_a3 htm adwft_al htm adwft_a2 htm adwft_b htm file C ADHOCw HELP adw_man htm 1 of 4 15 02 02 09 35 07 ADHOCw Users manual adwft_c htm adwft_d htm gt page 6 of adhocman doc 4 Program ADw2D coloured paper if possible adw2d htm adw2d_a htm adw2d_y htm adw2d_b htm adw2d bt h adw2d_c ht adw2dd1t adw2dd2t adw2d_d h adw2di2t h adw2d_f h adw2d_e h adw2di3t htm landscape printing inserted after the page 1 of adw2d_e htm adw2di4t htm landscape printing inserted after the page 2 of adw2d_e htm adw2d_k htm adw2d_kt htm adw2d_k1 htm adw2d_k2 htm adw_uspa htm gt page 7 of adhocman doc 5 Program ADw3D coloured paper if possible adw3d htm adw3d_z htm adw3d_e htm adw3d_a htm adw3d_1t htm adw3d_b htm adw3d_c htm adw3d_et htm landscape printing inserted after the page 1 of adw3d_c htm adw3d_f htm adw3d_g htm adw3d_h htm adw_uspa htm gt page 8 of adhocman doc 6 Program ADwT1 coloured paper if possible m landscape printing inserted after the page 1 of adw2d_ b htm m landscape printing inserted after the page 1 of adw2d_c htm landscape printing inserted after the page 2 of adw2d_c htm m landscape printing BBG CGE SC landscape printing inserted afte
221. cw help adhocw htm file This file is adwt1_fc htm file C ADHOCw HELP adwt1_fc htm 2 of 3 15 02 02 09 34 29 ADwT1 function menu window Return to main ADHOCw menu Return to main ADwWT1 menu file C ADHOCw HELP adwt1_fc htm 3 of 3 15 02 02 09 34 29 ADwT1 Other ADP directory ADwT1 Return to main ADwT1 help Creating files with different dimensions Some functions like C10 build custom made lambda cubes B10 extraction of a sub cube or a sub image F02 TIGER or G01 PYTHEAS will create output files with dimensions that are different from the current ones But the basis of ADHOCw if to have only an ADP parameter file with specific dimensions in one directory In this case the functions will manage the possibility to create the output data file s in a different directory and to create here also a new ADP and ADQ parameters file When the user will click on the Choose file button of the output file in the function menu the following window will appear file C ADHOCw HELP adwT1oth htm 1 of 4 15 02 02 09 34 30 ADwT1 Other ADP directory ADHOCw parameters You cannot in this case create the output file in the current directory You must detine or create a new directory where the output file will be created and where a new parameter file will be also written with ne new dimensions jE ADHOCws _plus BLAISOUS Open directory Choose file y Return to previous
222. d 171 5 294 78 190 144 area 1 241 445 171 2 349 0 area 2 355 340 361 307 area 3 999 0 0 0 area 4 999 0 0 0 area 5 999 0 0 0 area 6 999 0 0 0 area 7 999 0 0 0 area 8 999 0 0 0 area 9 999 0 0 0 area 10 999 0 0 0 area 11 zones Possible input for numerous ADHOC functions The output ADX ASCII file is a file which will be used further for the photometric correction It has the following structure 1 01887 13 9705 channel 1 A and B for Y AX B 1 15851 7 95754 channel 2 A and B for Y AX B 1 08544 3 47297 channel 3 A and B for Y AX B 1 29321 10 4741 channel 4 A and B for Y AX B 1 1239 9 61532 channel 5 A and B for Y AX B 1 21228 2 67023 channel 6 A and B for Y AX B 0 987761 9 15051 channel 7 A and B for Y AX B 1 16882 7 52532 channel 8 A and B for Y AX B 1 20114 2 72319 l hannel 9 A and B for Y AX B 1 23074 7 10736 channel 10 A and B for Y AX B 1 10415 8 04011 channel 11 A and B for Y AX B 1 02561 5 41701 channel 12 A and B for Y AX B 1 12552 15 8557 channel 13 A and B for Y AX B 1 00803 0 12065 channel 14 A and B for Y AX B 1 12978 1 28688 channel 15 A and B for Y AX B 1 13325 2 65948 channel 16 A and B for Y AX B 1 17313 10 0865 channel 17 A and B for Y AX B 1 21033 0 606203 channel 18 A and B for Y AX B 1 04791 7 43938 channel 19 A and B
223. d Velocities are necessary to compute the correct radial velocities maps The mean velocity of the objects allows the program to compute at every pixel the best interference order avoids modulo and the heliocentric radial velocity correction is relative to the date of he observation and the position of the object This last value can be computed in the menu A of the program The image scale is useful for complex functions as dynamics It can be changed at any time and many functions don t use this value which can be let to 1 at the beginning Examples of ADP or ADQ ASCII files Dummy object 512 1x dimension X 512 ly dimension Y 27 lz dimension Z 1 ixO corner X 1 iyO corner Y 1 iz0 corner Z 1 modefp 1 PF 2 spectro 1162 p PF interference order 6562 7797852 xlp lmd reference p 6598 9531250 xleta 1lmd calibration line 6598 9531250 xlbeta Imd calibration scan 6562 7797852 xlneb Imd zero object 6571 6401367 xlbneb lmd object scan 5 6454387 xil spectral length interfringe in Angstroems 6560 0000000 x11 Imd channel 1 0 0000000 vrO mean RV of the object in km s 0 0000000 corrv heliocentric correction to add to measures in km s 1 0000000 echelle scale pix 257 5000 xc center rings X file C ADHOCw HELP adwt1_ad htm 3 of 5 15 02 02 09 34 20 ADwT1 ADP parameter files 262 5000 yc center rings Y 1 0000000 ellipt X Y pixel ratio 0 mode_c mode center ellips of rings 0 normal
224. dual micro lens A0 301 ADw PYTHEAS creation of wavelength cube joj x 7 x EAS creation if ie FE Wave aie mee t CULE firs function can OY ran afer the Fi FIGEA IRC 1 Spectra position parameters Intput PYTHEAS coefficients from function F02 D Putheas SHISAPYTHEAS coefficients ADH Choose file 2 Calibration parameters Input 30 calibration spectra file Choose file LE Pytheas SH1524P039 ad3 3 Object parameters Approximated interference order p eoa a 6562 78 Angstroems Dorit compute exact interference order and use approxinjated order Scanning wavelength for calibration and object SRI Angstroems Input 30 observation file Choose file D Pytheas SH152 P038_ no COSMICE ad3 4 Sampling parameters Starting wavelength Angstraems 6520 0 o0 661 0 00 M Integrate pupil spot along the spectrum Ending wavelength Angstroems Wavelength step Angstmoens Reference object line for kinematics Hoian Angstroems 5 Result file CIADHOCw HELP adwtt_gt htm 2 of 14 15 02 02 09 34 35 ADwT1 PYTHEAS 1 PS SE a a a a M O 22 STS TTS 5 Result Output 3D wavelength file ae D Pytheas SH152 pytheas sh152 pytheas ad3 Output ADP parameter fle detined with the output 30 file D Pytheas SH152 pytheasish162 pytheas adp Output TAT verification file zero wavelength calibration interference order D Pytheas SH1 2ipytheas PYTHEAS zero wi Tat Output 20 ve
225. e CI ADHOCW HELP adw3d_f htm 2 of 3 15 02 02 09 34 16 ADw3D loading phase Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_f htm 3 of 3 15 02 02 09 34 16 ADwT1 phase computation ADwT1 Return to main ADHOCw help Return to main ADwT1 help C01 Computation of the phase The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page AD phase Of x ADHOCW 9 Stace computation favelength ot the channel 71 selective ceetor Inpu D his eatbiabon Choose ie e 6560 00 Angstroems note min 0 800 Output 27 fie eugh phase az test _Lood Mid spectrum B568 000 A angie max 360 000 AANHOC ws ji AT AISONSP as In 11 AN Load Calibration 6694453 A A Rmin 0 10 Output 27 fe parabaliz passe usse or eductons Chaise fie Geometry fassan AADHOCWS plus BLAISOUSThes prb AD2 Centar of ringe ee Output 2 fle tact 2am of al tae salration channels o_o te 26250 rotilge nn el AADHOCWS_plus BLAISOUSISUM_cal AD2 Plketratioxsw reongo amp D Noh al 2 fel Reli eh iishi an aklni Choose tae M xr forced to 1 CCD P Nb of chnis AADIOCNS_pius BLAISOUSRV cal AD2 C imle aml dek olee C Fixes iuels Scanning parameters if eae anl elliplic y jo ee Interference order p jwz at
226. e Suppress Input 20 file 12 DAData Godboutcai20 ad2 Choose file Suppress Input 20 fle 13 baDataiGodboutical21 a82 Choose file Suppress Input 20 file 14 baDataiGodboutical21 a82 Choose file Suppress Input 20 file 15 p Data Godboutical22 ad2 Choose file Suppress amp Horizontal cross section Line 240 toline 240 Starting column 35 Ending column 154 file C ADHOCw HELP adwt1_h4 htm 1 of 4 15 02 02 09 34 59 Input files format ADwTI1 tuning amp Horizontal cross section Line 240 toline 240 Starting column 25 Ending column 151 Vertical cross section Column ni to column Starting line az Ending line Box analysis xi fams Y1 az To ne Y2 This program gets horizontal vertical cuts or a box analysis in order to tune the instrument Up to 15 2D files are analyzed The user must first decompose the 3D file into 2D slices see the ADwFT slice function Cuts are useful to tune interferometer one can see different profiles corresponding for instance to different optical tunings The half maximum width is drawn Box analysis is useful to get the focus on the telescope the seeing is computed When giving the 2D input file names if the first 01 name is in the format Znnncckk where Znnn is the identification cc is the cycle and kk is the channel with extension ADA AD2 FIT or FITS the following file names will be automatically incremented HO call 2 ad 02 call 3 ad
227. e ADWIPCS EXE directory CCIR_N DCF 256x256 non interlaced Thomson camera CAD41K1T DCF DALSA CAD4 camera for AsGa Matrox driver for control display is a VCF file indicating the monitor driver for the control monitor plugged on the Matrox board The following VCF files are normally present in the ADWIPCS EXE directory VM101_60 VCF 640x480 60 Hz not recommended file C ADHOCw HELP adwi_a htm 4 of 7 15 02 02 09 34 00 ADwIPCS Parameters VM101_72 VCF 640x480 72 Hz not recommended VM103_60 VCF 800x600 60 Hz OK for Thomson or DALSA 512 VM103_72 VCF 800x600 72 Hz VM105_60 VCF 1024x768 60 Hz OK for Thomson DALSA 512 or 1024 VM105_72 VCF 1024x768 72 Hz VM107_60 VCF 1280x1024 60 Hz VM107_72 VCF 1280x1024 72 Hz VM11C_60 VCF 1600x1200 60 Hz VM11C_72 VCF 1600x1200 72 Hz WARNING THE ADWIPCS PROGRAM NEEDS TO HAVE A CONTROL MONITOR ACCEPTING IMAGES OF THE SAME SIZE THAT THE DETECTOR If not there is a Matrox MdigGrab error Thomson needs at minimum 256 vertical lines DALSA AsGa 512x512 needs at minimum 512 vertical lines DALSA AsGa 1024x1024 needs at minimum 1024 vertical lines HOW TO CHECK THE CAPABILITIES OF THE CONTROL MONITOR load a DEF file with the VCF chosen driver press the Check Matrox PF key ask for Single message on screen if the OK message is visible this means that the monitor accepts this driver i e the dimensions and scanning rate which are specified
228. e all beginning with two slashes followed by a space and ending with a semi colon preceded by a space Example This is a comment Note the necessity of the termination by a Example of a batch ASCII file The following file was obtained from the Store macro button and edited by a common text editor This is an example of a batch file for ADHOCw blank lines are neutral SUM3D2D fin D ADHOCws_plus BLAISOUS Oba da3 fout D ADHOCws_plus BLAISOUS toto ad2 smoothing operation SMOOTHXY fin D ADHOCws_plus BLAISOUS Oba da3 fout D ADHOCws_plus BLAISOUS toto2 ad3 square 3 phase computation PHASE fin D ADHOCws_plus BLAISOUS Call da3 ph_bru D ADHOCws_plus BLAISOUS Phas_bru AD2 ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 cal_sum D ADHOCws_plus BLAISOUS Sum_cal AD2 cal_rv D ADHOCws_plus BLAISOUS Cal_RV AD2 x11 6560 000000 xc 257 50 yc 262 50 ellipt 1 00 center 1 elliptCCD 0 p_pf 1162 Imbd_p 6562 780 Imbd_cal 6598 953 Imbd_scancal 6598 953 Imbd_obj 6562 780 Imbd_scanobj 6571 640 minangle 0 000 maxangle 360 000 minradius 0 000 maxradius 99999 000 end of the batch file file C ADHOCw HELP adwt1_ba htm 5 of 6 15 02 02 09 34 07 ADwT1 batchs Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HT
229. e cycles are scanned in increasing mode See saw mode decreases the effects of transparency and seeing variations over the observation This mode is recommended The ADw3D program manages the waiting of the channels in every case The dialog window appears as ADHOCw Origin of the data cubes Code of the observation Cycles to integrate Indicate here one of the input data files Choose file Start cycle f End cycle 9999 5 iS ADA files 2 bytes coordinate oi IV Seesaw mode for scanning usually checked Pains ob the onguval PRE scanning alternatively channels 1 gt n and n gt 1 Dimx 256 Dimy 256 Nbchannels 24 H Normally DimX 256 and DimY 256 Bin ning 1x1 C 2x2 C 4x4 C 8x8 C 16x16 X Cancel 7 Help CIG or TRI files these photon counting files are issued from the photon counting acquisition working at the 6m SAO telescope Russia and are similar to IPCS 4 bytes ADA files The dialog window appears as file C ADHOCw HELP adw3d_z htm 2 of 4 15 02 02 09 33 58 ADw3D acquisition modes 08 ADw ADA format Pile Es ADHOCw Origin of the data cubes M Code of the observation q Cycles to integrate Indicate here one of the input data files Choose file Start cycle 1 End cycle 9999 TRIM files Dimensions of the orginal image DimX 512 Dimy 512 Nbchannels 24 rs Usually DimX 512 and DimY 512 i Binning
230. e macro The user must only give the name of the 2D input and output files The computation is the following the parabolic phase value gives the new value by computing the modulo of the number of channels Than as the old ADHOC DOS specification the value is multiplied by 100 because it will be recorded as an integer The original null values are set to old ADHOC null values 32768 The input file can be of new ADHOCw type AD2 or old ADHOC type DA2 The output file is created as old ADHOC type DA2 file C ADHOCw HELP adwt1_h2 htm 1 of 3 15 02 02 09 34 18 ADwT1 translation of the phase to old ADHOC format This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example OLDPHASE fin D ADHOCws_plus BLAISOUS Phas_prb AD2 fout D ADHOCws_plus BLATISOUS Phas_org DA2 keyword content options OLDPHASE fin parabolic phase 2D input file name with whole path fout old ADHOC phase 2D output file name with whole path Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser i
231. e mouse Cross sections Integration of profile nes modification a Le He Mini 163840 000000axi 1035 000000 Cross section parameters Thickness 1 0 pixels ADw2D image modifications ADw2D Return to main ADHOCw help Return to main ADw2D help Image modifications This mode allows the modifications of the 2D image itself The user must change first the Action of the left button of the mouse to Image modification In this case the right part of the window will appear like this r Modification of mage file 07 This operation is excl bel for 20 ce 01 Replacement operation Arya f 3 Ea Set Value to HULL Undo 2D successive modifications Click fet mouse bution to rodily image Area modified is given by the cursor size in the zoom Presenthy fi g pix M Extend modification on the lett Extend modifications on the right Extend modifications on the top PF Extend modifications on the bottom Save modified 2D file 1 Note that you can only modify the image 01 The other possible superimposed 2D files will remain unchanged file C ADHOCw HELP adwa2d_f htm 1 of 3 15 02 02 09 33 53 ADw2D image modifications One important thing is to know that the cursor size in the zoom area gives the brush of the modification If the cursor size is for instance 7x7 pixels 49 pixels will be modified at the same time Modification procedure when pressing the left button m
232. e phinn AIT eny j LIL LINE ax Wind LISTE r tetmeoucernon ETRE raa CN vont Sommet 3 LRU CE LELED d SCENE di T Asti peor gt rarasncirg Iyp at apine ype absence Ct anaya eo RLS 30 calibration Random simatstion Sn TEA ADHOC Era man pmnanh aoe w IW owib du obtet Current LL fer fi ENS COTRTRA LE DTTLL LS au fau fiu wo f emposuretdme per channel isacords LE P fn fa 1 COUCOU ICE el ghee esognss 3562 780 panan stamnung wavelength Al SDobject ahm tingrinmin t none Lideniific ation ter eue dara and og file names th ihe observation number La nt Tea Case ts EXT eee Aant Mim amia prena dl baar ar Thee aiea ene Joyla mke eH gya d Poste Fad my aa mi na EE s Kaem gy poe tyme Srann HOT jatunmi C Simy aila PAB n amle Scanrang sorArolar Chtt mAnrtaca C Porallet sc him T Seria R222 CHAS Four C Test tie Disk scorege Maron board error contrat Baiser 1 LE eut errr ICTACTET 7 i ite mse Kant Y 255 256 2 hates X us Printthe werdiow goste Mistroa H Tune THT t Usts tila nemos Pick ADA tshi file namne LULU ce bata Saleem te LT Sh AO Li Obacrection ing Me CASE ADT file C ADHOCw HELP adwi_a htm 1 of 7 15 02 02 09 34 00 ADHOCw photon counting acquisition parameters Lord GISP to ruent 1 re nmana uf fh lean mili migun ce g Iann Minii fi starting cycis number l Aha preter sea character trom A 1o 2 when wll b
233. e totally parametrable Additional curves Pressing the Add TXT curve button opens the following window AD ADw2D added curves OI x ADw2D adding curves on the kinematical graph The user may superimpose up to 3 curves from outside ASCII files These curves can be previously published curves ex HI data or analytic computation curves or any curve to superimpose to the reduced data graph The input TXT ASCII files must have one line per point Each line is free formatted and has at minimum 2 values X and Y is the radius position while Y is the velocity Add the following curves just once now C Add the following curves every time the graph is drawn C Don t draw the following curves Scale fi 0000 arcsec image pixel File name Drawing Color Symbol Symbol size Line width Unit Curve 01 Courbe tt Symbols a Fuchsia Filed square 7 3 2 arcsec Change Curve 02 No Fuchsia Filed square x 4 2 arcsec Change Curve 03 No x Aqua x Filled square 4 2 arcsec gt Change file C ADHOCw HELP adw2d_k1 htm 6 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph Change and then displays a similar graph Kmjs 300 200 100 100 arcsec Additional functions Superposition of a mean curve Draw a polynomial curve the user can superimpose a polynomial curve For this he must check this box Imp
234. e used tor thin che scams 20 Image los 0 ot quire and phare aingie 20 imone inthis Hie evens Medic LD ed plua al ee TIE eet cc reared ae appare chanel are conne in order 40 Mot similar dep n may semal Sis iiu feat ad ET gnam i ees veil bese Oh ed ee uf TE pesudo number ot charms he Peoudo eapoeurs time per channel the paruo rambet of cpeice tohing In achourt dating Khama amil opie Kl a AH R e pladas in tappa sme Lone of course superimposed LEE EE ALGILT TETTI ATE DIE Hee nite FY invel I iwar THT pean Tit AI LL ET 1 LL TL i paralci Losd Chilre current NOF forthe ecqufekion parameters Type of scquserteon AF aaalilu inn inilir PTE CEE TETE eana ES Qu object inthokene the darma CIC Etang parameiore Iya werent TW IPCS integraces the direct phocon courir TY RETOE DILE LUE imn biu h alia aha l dhiul m The gpr ina bos named random rubar of pointe inceceta tha number ot ADwIPCS Parameters Identification The number of the observation can range between 0 and 999 The prefix is a character from A to Z which will be used for the data and log file names with the observation number The comment is written in the observation logbook with the timing of the scans The observation number increments automatically at every run Pressing on the Test button sets the prefix to T Type of acquisition 2D image allows to
235. ease the size of the photon addresses witch can be binned later by software For Thomson this value is 256 Stored image Y size is the size of the recorded photons Y addresses For DALSA AsGa it is usually the same value that CCD Y size there is no interest to decrease the size of the photon addresses witch can be binned later by software For Thomson this value is 256 Frames per second is used to compute the elementary exposure time and also the photon counting efficiency based on the frame count This value is 25 for Thomson 40 or 80 high rate for DALSA AsGa 512x512 and 20 or 40 high rate for DALSA AsGa 1024x1024 High rate DALSA AsGa is obtained via a switch on the DALSA camera itself ADw3D binning display allows to the display program ADw3D called by ADwIPCS to bin observations for quick look This function is interesting for 1024x1024 in order to get sufficient S N for the display If there is no binning put the value 1 DALSA high rate swap indicates to the program to correct the addresses with a X swapping in the right part of the image for DALSA AsGa camera This is due to the fact that the high rate frames per second doubled uses 2 output devices and that the second produces a X mirror effect For DALSA AsGa high rate frames per second put 1 For all other cases put 0 Matrox driver for camera is a DCF file indicating the acquisition driver for the camera The following DCF files are normally present in th
236. ected only if the 2D values of the image mask are inside the 2D value range Select 20 hile file C ADHOCw HELP adwt1_ma htm 1 of 3 15 02 02 09 34 16 ADwT 1 execution mask The execution mask is available for functions when it is possible This mask allows the operation on ly on specified pixels channels or values You can include a rectangular area by default the maximum area You can exclude a rectangular area You can include channels Bounds are included 19 6 is the inverse of 7 18 If the second channel value k2 is smaller than the first channel value k1 this means that the channels k2 to k1 though 1 are selected You can include values By default the maximum range 3 1E 38 to 3 1E 38 is taken For 2D files this is the value of the pixel For 3D files this is the value of the channel You can also use an image mask This image mask is a 2D image and operation is done only if the value is inside the given fork An operation is done if all the conditions are true at the same time Macro definition When you request a mask additional parameters will be add to the macro if they are not already defaults in this case they are not mentioned Example maski_x1 2 maski_x2 2 maski_y1l 250 maske_y2 250 maske_x1l 11 maske_x2 11 maske_y1 21 maske_y2 21 maskf D ADHOCws_plus BLAISOUS Zphasprb ad2 maskf_v1 100 maskf_v2 300 keyword content options maski_x1 included area x1 corner
237. ections ADwT1 Return to main ADHOCw help Return to main ADwT1 help H05 Various cube peculiar corrections F ADw Peculiar corrections ADHOCw Peculiar cube corrections hput 30 file Output 35 file Choose file C Megantic HP IB scanning shift 1 gt nbchn 2 Megantic HP IB scanning interpolation gt nbchn 2 rs Execute Help X Abort ESR store macro This program corrects peculiarly cubes Megantic scanning shift lf half is the half of the number of channels and number is the number of channels channels 1 to half 1 remain unchanged channels half to number 1 are shifted half half 1 half 1 half 2 22 channel number is interpolated number 1 1 2 Megantic scanning interpolation file C ADHOCw HELP adwt1_h5 htm 1 of 3 15 02 02 09 35 00 ADwT1 Peculiar corrections If half is the half of the number of channels number is the number of channels and k is the number of one given channel channels 1 to half 1 remain unchanged channels halfto number are interpolated as following a 13 5 13 54 11 1 2 b a 1 a k half float number half value of k value of k b value of k 1 1 b This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network
238. ed acquisition from CCD FITS acquisition FIT files 1060 514 7 interlacing 2 7 X Abort Help Principle The program can read already built cubes if they are in AD3 or DA3 format The program can also integrate observations In this case a background task is running in order to integrate 2D channel images slices as soon they are created by the detector acquisition system If the user wants only to integrate previous observations this task is running at the beginning and is simply waiting indefinitively If the program is called automatically from ADwIPCS the ADwIPCS program indicated to the ADw3D program the possible parameters of interlacing channels numbers are not continuously scanned but are interlaced with a factor 2 or 4 IPCS 256x256 this mode can be used during photon counting observations or later to integrate back already done observations The program ask for one of the existing channel ADA photon file From this basic file it is able to read the ADT acquisition information file This ADT information file gives important informations on the interlacing for instance and the program will be able to integrate the successive ADA files in the order they were produced One ADA file has a simple name Xnnncckk ADA where X is a literal character G for Ghasp for instance nnn is the observation number from 000 to 999 cc is the cycle number or scan number 00 to 99 and kk is the channel number 00 to 99 Extended
239. ed from 1 The input file can be of new ADHOCw type AD2 or old ADHOC type DA2 The output file is created as new ADHOCw type AD2 This function can use an execution mask When the execution mask doesn t allow the operation the cube value remains unchanged file C ADHOCw HELP adwt1_b3 htm 1 of 3 15 02 02 09 34 38 ADwT 1 insertion of a channel This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example INSERT2D3D fin D ADHOCws_plus BLAISOUS Call_ch8 AD2 fout D ADHOCws_plus BLATISOUS call_new ad3 chnl 8 r keyword content options ANSERT2D8D Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present file C ADHOCw HELP adwt1_b3 htm 2 of 3 15 02 02 09 34 38 ADwT1 insertion of a channel HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw he
240. eix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b10 htm file C ADHOCw HELP adwt1b10 htm 4 of 5 15 02 02 09 34 31 ADwT1 sub subes or images Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1b10 htm 5 of 5 15 02 02 09 34 31 ADwT1 TIGER 2 ADwT1 Return to main ADHOCw help Return to main ADwT1 help F02 TIGER creation of the 3D wavelength cube How to reduce TIGER Function F02 This function is the second step for TIGER and PYTHEAS data reductions after F01 This function created a new cube in a new directory with new dimensions Procedure 1 the program computes the dispersion curves for every micro lens spectrum 2 then the program rejects spectra from the calibration position and the dispersion polynomial 3 and builds the output 3D file following the output geometrical sampling The result is in a different directory because 3D dimensions are different from the input To check after execution nb rejected spectra from sigma position log information nb total of calibration verification
241. ending execution message the following information is recorded 0238 O01 Lower 14 18 34 Beginning step 1 opening creating files file C ADHOCw HELP adwt1_c1 htm 5 of 6 15 02 02 09 34 17 ADwT1 phase computation 2 19 14 Measured 262092 262144 not masked pixels Y X pixel ratio Shift calibration from 6598 9531 A computing the rough phase 100 0 computing the center of rings ix1 ix2 iyl iy2 146 369 151 374 X 258 5 Y 263 5 ratio 1 00000 checked and found to be was checked and found building the parabolic curve 3 18 at mean r 1 3 12 pixels computing the parabolic phase computing scanning corrections 6559 2339 A 3 6640 channels correcting the parabolic phase correcting the RV calibration 0238 01 Lower 14 18 37 Beginning step 2 0238 01 Lower 14 0238 Ol1 Lower 14 19 14 Beginning step 3 0238 01 Lower 14 25 03 Detail centers 0238 O0 Lower 14 25 03 Center of rings 0238 01 Lower 14 25 03 Ellipticity Y X pixel 0238 01 Lower 14 25 03 Center coherence was correct less than 20 pixels deviation 0238 01 Lower 14 25 03 Ellipticity to be correct less than 10 deviation 0238 01 Lower 14 19 14 Beginning step 4 0238 O01 Lower 14 19 15 Phase center 0238 Ol1 Lower 14 19 15 Beginning step 5 map 0238 01 Lower 14 19 57 Beginning step 6 0238 01 Lower 14 19 57 to 6560 0000 A 0
242. ensifier and get P rot Fabry rings Run the Move and test the PF interferometer test Change channel number and press on the Move PF button If the diameter of the ring is changing it is OK If not you have an hardware problem Is the CS100 on Is the CS100 connected to the computer 4 get the TV acquisition parameters Tune THT get a photon counting flux Press the Acquire 1 frame button of the Grab image and identify photons test The program displays the image and the counted photons as crosses on the second VGA display The Black level and the White Level define the limits of the Matrox digitalization The Discri is not independent of the Black Level You must obtain the counting of the apparent photons Display source displays the TV frame Display binarization displays the binarized frame that is used to count photons Display positions displays counted photons as crosses If the number of crosses is high you can stop their drawing by pressing the Abort crosses display button The Discri Black level and White Level are critical If you change the THT these parameters varies store the TV levels as custom values for acquisition i e transfer these values to the acquisition parameters Warning this is not automatic If you forget old parameters will file C ADHOCw HELP adwi_e htm 2 of 4 15 02 02 09 34 04 ADwIPCS tuning be used Check frequently the TV acquisition para
243. ensions Ix 1512 Wy 1512 le 27 Mouse profile area fist pix X By Printer setup B Print screen i Save 3D data Help Z Save to BMP mR Save to BI x E X Guit the program Y ay Value RE PA Channel lt 1 a Waiting gap sec EE General Statistics Phase Sum Interferograms Wavelength maps Mono cont AY Display parameters ett Rainbow Scale max 16160 Threshold 0 1 1 10 10 100 100 1000 1000 Channel 21 Channel 22 Channel 23 Channel 24 Step 1010 4 4 10 10 400 100 000 1000 gt i 4 Scale min 0 Channel 25 Channel 26 Channel 27 M Scale overlap file C ADHOCw HELP ADw3D_1t htm 1 of 2 15 02 02 09 34 12 ADw3D interf full size file C ADHOCw HELP ADw3D_1t htm 2 of 2 15 02 02 09 34 12 ADw3D main 2D display screen ADw3D Return to main ADHOCw help Return to main ADw3D help Main 2D display screen Sum This mode corresponds to the Sum folder The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page DIIOUw JU display mun panci Gains fs fs Lh rap AR DURE Birvi 73 F Es LP TT PP ECG Xe Landes few he den Detengef esse ietvari Heed y ino rtoragram channel 1 isplayed l im Fate tet AL alte Irv wurye
244. ent lines at the end For instance the following file which is coming from an old ADHOC sequence is valid 35 23 245 101 Zone 1 280 353 532 475 Zone 2 4 175 500 207 Zone 5 5 249 302 351 Zone 7 143 313 241 389 Zone 9 143 453 143 453 Zone 11 0 00 0 Zone 3 000 0 Zone 4 0 0 0 0 Zone 6 0 00 0 Zone 8 0 00 0 Zone 10 O99 999 999 2099 Zone 0 zones Possible input for numerous ADHOC functions but new files with floating coordinates as the following are also valid 171 5 294 78 190 144 area 1 241 445 171 2 349 0 area 2 355 340 361 307 area 3 ADHOCw zones x1 yl x2 y2 You can use a reference photometric 2D file which is supposed for example to give an idea of the flat field through the filter instrument detector If this file is absent the reference values are considered to be 1 If the reference 2D file has null values they are not taken in account the sum of the profile is not incremented The recommended recurrent substraction is 1 pass with a substraction factor equal to 1 More sophisticated OH suppression can use the multi pass algorithm You can suppress also the continuum at the last pass at the continuum level you decide If the checkbox Use the rough OH profile is checked the program will run immediately and simply integrate the OH profiles in the zones If the checkbox build and correct interactively and graphically the OH profile box is checked the program will first compute the profile
245. erations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_a1 htm Return to main ADHOCw menu Return to main ADWFT menu file C ADHOCw HELP adwft_a1 htm 2 of 2 15 02 02 09 34 08 ADwET files structure ADwFT Return to main ADHOCw help Return to main ADWFT help File structure information minimum and maximum You can get a full information of the 2D or 3D data files The file format is automatically recognized Eo ADWFT Pale kei aT scale la A 10 ADHOCw File Translator ssion100 Jex Presentation 3D gt 3B 2D gt 2D 3D gt 2D slices 2D slices gt 3D File parameters Dump and modify Macros ppi 96 Functions This function detects the type of an input data file Structure parameters dimensions ordering are listed as well as the fle comment If the file is written in FITS one can list the header If the file is written in ADHOCw format one can list and modify the different parameters It is also possible to request the search of the minimum and maximum values of the file Possible normalization of conversions new_value old_value B ls f 0 B 0 0 About Help XM Quit File Translator Information on a data file file C ADHOCw HELP adwft_b htm 1 of 6 15 02 02 09 34 08 ADwFT files structure By pressing on the Information on
246. erpolating profiles The operation can be re iterated dialog box number of iterations WARNING For CCD cosmic rays suppression the operation must be executed on the original 3D files directly taken from the observation If there is any smoothing dephasing interpolating operation the abnormal pixel value is smoothed Specially if dephased the unique abnormal channel value pollutes the adjacent channels The contrast of the wrong value is diminished and the B12 ADwT1 function is no more efficient The input file can be of new ADHOCw type AD2 or AD3 or old ADHOC type AD2 or DA3 The output file is created as new ADHOCw type AD2 or AD3 This function can use an execution mask When the execution mask doesn t allow the operation the extracting value is set to a null value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example SIGMA fin E ADHOCws_plus BLAISOUS Oba da3 fout E ADHOCws_plus BLAISOUS bidon2 ad3 oper 0 deriv 1 sigma 5 iter 2 keyword content options SIGMA fo fin 3D input file name with whole path fout 3D output file name with whole path file C ADHOCw HELP adwt1b12 htm 3 of 5 15 02 02 09 34 44 ADwT1 sorting eliminating interp
247. ers from rough analysis of non dephased channels Continuum substraction from given areas Execute a function Quit the program gui tne progrm 7 Help Session log book see the ADL log file for the full history of all the sessions F Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions For that press the Show logbook button above at any time You can also edit a batch file by pressing the Exec a batch file button You will get the following window file C ADHOCw HELP adwt1_ba htm 3 of 6 15 02 02 09 34 07 ADwTI1 batchs ADHOCw macro file edition Macrofie D ADHocws_plusiBLAISOUS toto adm All the macro files are ASCII files and have the extendion ADM Save file The easiest way to write macros is to use the normal dialog of the functions and to choose Store macro instead of Execute In this case you may store the macro in a a i new or existing macro file append You can also edit the ADM file with a common ASCII editor Help SUM3D2D fin D ADHOCws_plus BLAISOUS 0ba da3 fout D ADHOCwS_plus BLAISOUS toto ad2 SMOOTHXY fin D ADHOCwS_plus BLAISOUS Oba da3 fout D ADHOCwSs_plus BLAISOUS toto2 ad3 square 3 PHASE fin D ADHOCwSs_plus BLAISOUS Cal da3 ph_bru D ADHOCws_plus BLAISOUS Phas_bru AD2
248. erving arrays 0271 01 Lower 15 42 51 Reading ADS seeing file 0271 15 42 51 Building gaussian arrays 0271 15 42 51 Computing result Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c8 htm Return to main ADHOCw menu file C ADHOCw HELP adwt1_c8 htm 3 of 4 15 02 02 09 34 50 ADwT1 Return to main ADwWT1 menu file C ADHOCw HELP adwt1_c8 htm 4 of 4 15 02 02 09 34 50 AdwT1 wavelength computation ADwT1 Return to main ADHOCw help Return to main ADwT1 help C02 Computation of the wavelength cube nO 4 ADw wavelength maps ADHOCw LOGGER OF WAVE maps Input 30 file interteragrarms Choose file Input 20 parabolic phase Choose file D ADHOCws _plus BLAISOUS Phas_prb 402 Output 30 file wavelength maps Choose file Store macro The program computes a dephased cube from an observation cube and the parabolic phase map obtained from the function C01 The input files can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output file is created
249. eshold to separate the spectra EALLI Maximum spectrum length in pixels Maximum spectrum width in pixels Minimum spectrum length for elimination in pixels Minimum spectrum width for elimination in pixels 1 2 Geometric parameters from lens array This OPTIONAL STEP affows fo eliminate spectra which appear outside of fhe acre fenses positions Eliminate spectra on position coherence Output 2D eliminated spectra file after coherence elimination Choose file D Pytheas s H152 TIGER_eliminated AD2 Output 2D remaining spectra file after coherence elimination Choose file D Pytheas SH1 52 TIGER_selected AD2 3 Result for next TIGER or PYTHEAS step Output TXT spectra positions file Choose file D Pytheas s H152 TIGER_pos TXT va Execute Help x Abort EX Store macro file C ADHOCw HELP adwt1_f1 htm 2 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 1 Extraction parameters Input 2D continuum file in case of Pytheas this is the sum of all the continuum channels Output 2D verification file draws in superposition of continuum spectra the shape of the spectra which are found Displaying it with ADw2D with the same levels as for the continuum file will clearly show the different spectra and the corresponding shapes Threshold this threshold must be defined in order to separate TOTALLY the spectra use ADw2D to find this value Threshold too low confusion Threshold too high T
250. essed any kind channels 3 FITS any kind by spectra f32 f64 i8 i16 i32 4 FITS any kind by channels f32 f64 i8 i16 i32 5 ADHOCw by channels unusual PC or Unix f32 AD3 6 Binary or IDL PC int16 spectra 7 Binary or IDL PC float spectra 8 Binary or IDL PC int16 channels 9 Binary or IDL PC float channels 10 Binary or IDL Unix int16 spectra 11 Binary or IDL Unix float spectra 12 Binary or IDL Unix int16 channels 13 Binary or IDL Unix float channels outputtype for 3D files 0 ADHOCw PC default AD3 float32 spectral 1 ADHOC old VISU3 DA3 int16 spectra 2 EIC compressed SUN new int16 3 FITS 32 float32 spectra 4 FITS 32 float32 channels 5 ADHOCw PC float32 channels unusual 6 Binary or IDL PC int16 spectra 7 Binary or IDL PC float spectra 8 Binary or IDL PC int16 channels 9 Binary or IDL PC float channels 10 Binary or IDL Unix int16 spectra 11 Binary or IDL Unix float spectra 12 Binary or IDL Unix int16 channels 13 Binary or IDL Unix float channels 14 FITS 64 float64 spectra file C ADHOCw HELP adwft_d htm 3 of 6 15 02 02 09 34 09 ADwET Macros and batch 15 FITS 64 float64 channels 16 FITS 8 int8 spectra 17 FITS 8 int8 channels 18 FITS 16 int16 spectra 19 FITS 16 int16 channels 20 FITS 32 int32 spectra 21 FITS 32 int82 channels 22 ADHOCw Unix AD3 swapped float32 by spectra 23
251. et to a null value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example PHOTOM_CHNL fin E Al DHOCws_plus BLAI DHOCws_plus BLAI fout E A fphotom E A DHOCws_plus BLAI SOUS bidon2 ad3 SOUS bidon adx keyword PHOTOM_CHNL 3D input file name with whole path fin fout content SOUS oba2 ad3 options 3D output file name with whole path fphotom Log book results ASCII ADX photometric parameters file Excepted the text of the macro and the ending execution message the following information is recorded 0272 01 Lower 13 970500 0272 01 Lower 7 957540 0272 01 Lower 31305 Chnl 2 31 05 Chnl 2 31 05 Chnl file C ADHOCw HELP adwt1b15 htm 2 of 4 15 02 02 09 34 45 1 2 3 New A OLl New A OL New A OLl d d d B B B A A A 1 018870 B 1 158510 B 1 085440 ADwT1 Photometric corrrection B 3 472970
252. f ADwIPCS When the ADwIPCS acquisition program is executed the ADw3D display program is automatically launched The necessary parameters cube dimensions name of the ADA or FITS files interlacing are automatically transmitted to the display program The ADW3D program waits for the availability of the acquisition files there is one file for one basic channel exposure and updates immediately the 3D display In the left side upper corner there is a waiting gap box which allows to tune the minimum waiting time between the search of the next file This allows eventually to decrease the computer load Cube dimensions x B12 Is EE lz 27 Printer setup Print screen LS Save ID data Help 3 Save to BMP x Cut the program r e Wating gap sec file C ADHOCw HELP adw3d_ip htm 1 of 2 15 02 02 09 34 04 ADw3D_IPCS Return to main ADwIPCS help Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_ip htm Return to main ADHOCw menu Return to main ADwIPCS menu file CI ADHOCW HELP adw3d_ip h
253. float zoom zoom Note nbdim can be 2 3 or 3 2 2 D 3 3 D ordered in spectra Z X Y default for ADHOC 3 3 D ordered in channels X Y Z N A NO ND ND N TLE For 2 D files Mi 44 47 float thrshid last threshod 0 12 4751 float step llaststep 180 ote7 mused Note these values are just keeping the last displaying parameters as for VISU2 parameter files For 3 D files location bytes type mnemo description default 0 43 float xl lambda of the 1st channel in Angstroems 6600 12 47 51 ffloativro mean radial velocity of the object km s fo 13 52 55 floaticorv heliocentric RV correction km s ss 6 59 ffloat jp0 PF interference order 793 FR FR A O1 file C ADHOCw HELP adw_what htm 8 of 15 15 02 02 09 33 45 ADw what is ADHOCw 15 60 63 ifloat xlp reference lambda for pO in Angstroems 6563 16 64 67 float xl0 observed zero velocity lambda in Angstroems 6563 17 68 71 float vri radial velocity of the 1st channel in km s 0 18 7275 ffloat xik _ interfringe in km s 1386 19 76 127 lunused In Note these values are similar to 3 ADHOC VISU3 parameter files h Comments 128 bytes when read or written the 128th byte is automatically forced to O for C compatibility 2 Old ADHOC DOS Visu2 Visu3 format a structure des fichiers 2 D de type xxxxxxxx DA2
254. follow in order to recognize as a keyword Examples of an ASCII file containing macros examples converts an ADHOCw 3D file into a FITS channel channel file here no default directory was mentioned full paths are requested FILTRANS 3D3D tin 0 tout 4 fin d toto ad3 fout d travail essai tutu fit sets the default directory __ PARAMS dd d travail converts an old ADHOC image into a FITS 16 image FILTRANS 2D2D tin 1 tout 18 fin image DA2 fout image fit converts a binary image floats FILTRANS 2D2D tin 6 tout 0 Ix 100 ly 100 fin image idl fout image ad3 builds a cube from CFHT observations FILTRANS s3D tin 18 tout 0 nc 32 first 27 cfht 1 fin 3109 fit fout 3109 ad3 conversion with normalization FILTRANS 3D3D tin 0 tout 1 a 2 b 0 fin tutu ad3 fout tutu da3 Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwft_d htm 5 of 6 15 02 02 09 34 09 ADwET Macros and batch Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_d htm Return to main ADHOCw menu Return to main ADWFT menu file C
255. following PA is the mean position PA1 PA2 2 angle of the crown sector Vs is the systemic velocity of the crown sector incli is the inclination of the crown sector When selecting a pixel the computation is the following the crown sector is selected coordinates on the sky r gt rmin r lt rmax p gt PA min p lt PA max the p and 6 galactic coordinates are computed from sky coordinates p and 6 For this PA PA1 PA2 2 of the selected crown sector and i is the inclination of the selected crown sector then the velocity is computed as rotation velocities are Vrot x y Vrot p RV x y Vs p sin i p cos 6 radial velocities are RV directly coming from the 2D file 01 projected rotation is PR x y RV Vs p cos 8 Vs p The crown sector is selected from the position of the pixel on the sky The computation is done in galactic coordinates Optimizing When crown sectors are defined the user can optimize the best major axis MA system velocity Vs and inclination i within the deferent crown sectors For this press the Minimize PA r Vs r and incli r button file C ADHOCw HELP adw2d_k2 htm 7 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns Kinematics of galaxies Parameters file Load file example adk Save to file F automatic saving Rotation velocities C Fixed parameters Params r Edit a params r array T
256. for Y AX B 1 15636 5 36424 channel 20 A and B for Y AX B 1 27735 8 60345 channel 21 A and B for Y AX B 1 23585 6 18837 channel 22 A and B for Y AX B 1 0964 6 14029 channel 23 A and B for Y AX B 1 20471 1 42619 channel 24 A and B for Y AX B 1 10585 9 21237 channel 25 A and B for Y AX B file C ADHOCw HELP adwt1_c5 htm 4 of 11 15 02 02 09 34 46 ADwT1 photometry from OH l 1 28748 10 6678 channel 26 A an 1723693 7 11 7664 channel 2 For the computation it is possible to use a reference photometric 2D file which is supposed for example to give an idea of the flat field through the filter instrument detector If this file is absent the reference values are conspired to be 1 If the reference 2D file has null values they are not taken in account the reference sum of the profile is not incremented The user can create control BMP file for every channel But this operation increases largely the computing time The following picture illustrates this possibility witch is mainly a control CORREL_OH 07 03 1999 09 27 31 channel 8 15537 pixels real Hus integrated measured flux per physical channel measured ireal b a 621542 b 15 198458 file C ADHOCw HELP adwt1_c5 htm 5 of 11 15 02 02 09 34 46 ADwT1 photometry from OH The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DAS This function can be execute direct
257. for original values b multiplying coefficient for added values c transparent value x0 X virtual pixel position in final frame X displacement yO M virtual pixel position in final frame Y displacement Ix X dimension of the added file ly Y dimension of the added file Z dimension of the added file only of 3D Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwtib17 him Return to main ADHOCw menu Return to main ADwT1 menu file CI ADHOCW HELP adwt1b17 htm 3 of 3 15 02 02 09 34 54 ADwT1 menu PROFILES ADwT1 Return to main ADHOCw help Return to main ADwT1 help Profiles functions D 1 ADw ADwT1 Pile x Bring task manager to front ADHOCw ADwT1 Version 994 JBx Obs Marseille 1280 s 1024 96 ppi es 1pcs Tiger Pytheas miscen D01 3D profile decomposition D02 3D adjacent pixel correlation Edit a batch file lt 3 Exec a batch file Display control
258. formation boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c4 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_c4 htm 6 of 6 15 02 02 09 34 15 ADwT1 control display ADwT1 Return to main ADwT1 help Display control window Some functions create output graphics usually BMP files This files can be displayed later with classical image display programs Ex Paint but they are also stored in a temporary buffer which can be displayed or printed from ADHOCw itself even during the execution of the function For that press the Display control button on the right of the menu window just above the Execute button You will get the following dialog window ADw Control control graphs or 0 tion Nou can access ta this control by using the buttons below CL From this you can display print or save into a file the graphic If you display it you will get something like this file C ADHOCw HELP adwt1_di htm 1 of 3 15 02 02 09 34 15 ADwT 1 control display ImageControl SEEIN
259. front of the screen overlapping all other windows Other buttons print window prints the acquisition window see parameters opens the parameter window without allowing to modify the parameters just to see them write on logbook this function is very useful the user can write directly comments on the ADT logbook file during the observations The comments are written with time information and are mixed in the scanning log informations display logbook the user can display the content of the ADT logbook file Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwi_d htm file C ADHOCw HELP adwi_d htm 3 of 4 15 02 02 09 34 03 ADwIPCS acquisition Return to main ADHOCw menu Return to main ADWIPCS menu file C ADHOCw HELP adwi_d htm 4 of 4 15 02 02 09 34 03 ADwIPCS acquisition full size ADHO C Wi photon C ounting Version 1 po JB x oe ep eres Cycles and channels Acquisition THT intensifier channel exposure 00000 s per 0015 Start 10467 volts tune THT current channel 0000 0024 SS
260. ft to highest bits The 2 lowest bits represent the Matrox C80 CPU number which was used for the centroiding of the frame 0 to 3 The ADT file is a log file ADHOC Track which contains the information on the P rot Fabry scanning and on the Photon Counting acquisition timing hardaware position of the interferometer number of counted photons number of counted frames incidents during exposure user comments This is an ASCII file which is used by the E01 ADwT1 function in order to build the cubes from the ADA photon files Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_what htm file C ADHOCw HELP adw_what htm 14 of 15 15 02 02 09 33 45 ADw what is ADHOCw Return to main ADHOCw menu file C ADHOCw HELP adw_what htm 15 of 15 15 02 02 09 33 45 ADWwTI_task Return to main ADHOCw help Return to main ADwT1 help Task manager window The task manager window is the second windows appearing when the ADwT1 program runs At the beginning the task manager is empty 06 11 1998 20 32 54 01 termin
261. h 256 colors and 96 pixels per inch If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d htm Return to main ADHOCw menu file C ADHOCw HELP adw3d htm 2 of 2 15 02 02 09 33 57 ADw3D acquisition modes ADw3D Return to main ADHOCw help Return to main ADw3D help Acquisition modes for the original cube When running the ADw3D program the following window appears first ADHOCw 3D display Pile E4 ADHOCw 3D display from real time acquisition OR already acquired data J Boulesteix ADHOC cubes AD3 or DA3 files C IPCS real time or deferred acquisition 256x256 Thomson detector 2 bytes coordinate ADA files Sex Sie Frame record C IPCS real time or deferred acquisition ICCD 4 or 6 bytes coordinate ADA files 512 51 2 No x ADHOCw C Deferred acquisition from 6m telescope recorded photon files CIG or TRI files C Deferr
262. hanar tir Srey Oie Hore he ice A Gp Suns te Pda PIE Makale nur irs hi Erim matriz Sapia peria E 2 2 B OH M 4 0 D amp amp r r 7 CC nman FHA eno C Dercntzlan PAH 4000 C Smoothing Sl Smaal x C CT smh e trt file with user Una a han ver rit rera Lea stn slain sh 2h Tura LI U qf Laccute uep Os Le User moi zer cakes and sch refed tmosthivz nze a12 bac ue meine The smoothing filter values are displayed on the right part of the window If the patter is larger than 17 pixels only the central values are displayed The user can choose different pre defined smoothings square gaussian lorentzian 5 pixels patters or give its own file C ADHOCw HELP adwt1_b8 htm 1 of 4 15 02 02 09 34 40 ADwT1 spectral smoothing smoothing pattern from an ASCII user file At any moment the user can update the displayed values by pressing the Update matrix button and print the matrix by pressing the Print matrix button In addition an execution mask possibility is available Square mode it is a Dirac function with a width given in integer pixels Gaussian mode is a gaussian curve with a width given in floating pixels Values lt 1 of the maximum are considered to be 0 in order to minimize matrix size Lorentzian mode is a lorentzian curve with a width given in floating pixels Values lt 1 of the maximum are considered to be 0 in order to minimize matrix size Smoothing mode
263. he coherence of approx ellipticity 1 enforce the values of the ellipticity center mode for checking the center and ellipticity 0 check the coherence of approx xc yc and ellipticity 1 enforce xc yc and ellipticity values p_pf interference order or the interferometer order interference order or the interferometer the interferometer elliptCCD special CCD parameter nothing done i X Y 1 pp Imbd_p Imbd_p reference wavelength of p_pf 2 wavelength of p_ reference wavelength of p_pf 2 Imbd_cal wavelength of the calibration line i Angstroems Imbd_scancal scanning wavelength of the calibration i Angstroems Imbd_obj wavelength of the object line at zero velocity in Angstroems Imbd_scanobj scanning wavelength of the object in Angstroems minangle minimum minimum angle of the sector degrees minimum angle of the sector degrees the sector degrees maxangle maximum angle of the sector degrees minradius minimum radius pixels maxradius maxradius maximum maximum radius pixels maximum radius pixels algorithm algorithm to analyze the profile change fixed levels chg_chnis number of successive inversed channels i see Note 1 case of algorithm 1 percentage of measured channels in case of pc_mono see Note 1 algorithm 2 Note 1 chg_chnis and pc_ mono exclude themselves Log book results Excepted the text of the macro and the
264. he position angle PA pP 9 p and 6 are connected via the following equations tg 0 tan6 cosji p 6 cos8 cos8 amp where i is the inclination with respect to sky plane 0 if the galaxy is face on and 90 if the galaxy is edge on In the kinematical functions two important extensions are powerful for trained users full kinematical graph window and user made crown sectors and kinematical parameters optimization If the kinematics of galaxies radio button is clicked the right part of the windows appears like this file C ADHOCw HELP adw2d_k htm 1 of 6 15 02 02 09 34 24 ADw2D kinematical functions When the user press the redraw graph button the window screen will appear like this file C ADHOCw HELP adw2d_k htm 2 of 6 15 02 02 09 34 24 ADw2D kinematical functions EF ED ADHIK w 2D adm Udit N ETAT CR h th Sinn h c i o3 Dins DC erise 7 sd X e see Bos LE Mouse cise Caso dows 405 acon T2433 7 fre pe he race Sart dhe mu TE PRT matine fay iy ncus ttn AE kaor Wi DHEISE een iezen C riais tow f lovated i lohomcnch gt mpri tiagh sioe kx sh everas Raed nv RENTE DETTE z px s race ci Pa hrs fiesta l RE p M enaze cawas A ey rh Perreters te Lxi es pr Max Csestofis dr Le KE alee ce ve ES Sana dure pu ma a be mene c ien 1707 E x Aslam vey 14 l E ee
265. he seeing and displacements variations 2 from the variation of the phase map when correcting from the seeing variations This function can use an execution mask When the execution mask doesn t allow the operation the extracting value is set to a null value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example CORRECT_SEEING fin E ADHOCws_ plus BLAISOUS oba 2 ad3 fout E ADHOCws_plus BLAISOUS bidon2 ad3 fseeing E ADHOCws_plus BLAISOUS bidon ads ph_prb E ADHOCws_plus BLAISOUS Phas_prb AD2 oper 0 seeing_max 2 523 interp 1 file C ADHOCw HELP adwt1_c8 htm 2 of 4 15 02 02 09 34 50 ADwT1 keyword content options fins input SD file fout output 3D file corrected PO ph_prb input 2D parabolic phase fseeing ADS input file oper 0 seeing and displacement corrections 1 seeing correction only 2 displacement correction only interp a mode no interpolation nearest integer ie Spatial and spectral linear interpolations default Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0271 15 42 43 Creating output files 0271 15 42 51 Res
266. hoose site Eso Paranal Chile v 70d 24 10 00 24d 37 31 00 Save to BMP Local Time Universal Time LT UT F4 hours Help Check LT UT value can change with seasons da month f raph widt Choose graph date fig x october x 200 x 16 hours v NGC 7764 18 10 2001 A 23h 48m 49 80s D 40d 57 2 00 ESO Paranal Chile LT UT 4 h O2h 56mn gt 1 76 x Quit 4 air mass Log book results None file C ADHOCw HELP adwt1_h6 htm 2 of 3 15 02 02 09 35 00 ADwT1 Precessions Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h6 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_h6 htm 3 of 3 15 02 02 09 35 00 ADvwT1 sideral clock ADwT1 Return to main ADHOCw help Return to main ADwT1 help H07 Sideral Time clock O ADw Sideral Time T_ jor x ADHOCw Sigeral Time clack Longitude Latitude Site information Eso La Silla Chile Fod 44 45 00 23d 152400 Local Time Universal Time LT LIT 4 hours Check LT UT value can change with se
267. hreshold correct good file C ADHOCw HELP adwt1_f1 htm 3 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 separation Maximum spectrum length and width could be larger than the largest spectrum These values are used to reject wrong lines or outside defects Minimum spectrum length and width used in order to reject small defects 2 Geometric parameters from lens array This section is used optionally to reject spectra which could be outside the normal geometry of the lenses Usually it is not needed and is nor compatible with any geometrical distortion See below the description of this option 3 Output files Eliminated spectra file draws in superposition of continuum spectra the shape of the spectra which were eliminated from the optional geometric parameters Remaining spectra file draws in superposition of continuum spectra the shape of the spectra which remain after elimination from the optional geometric parameters Note all the final spectra are normalized to a common pixel height For all these files displaying with ADw2D with the same levels as for the continuum file will clearly show the different spectra and the corresponding shapes If there is no elimination from geometry the output 2D verification file and the output 2D remaining spectra file are identical Output TXT spectra position file this contains the information which will be transmitted to the F02 function to build cubes The file is TXT be
268. ick here for AD1 format file C ADHOCw HELP adw_what htm 5 of 15 15 02 02 09 33 45 ADw what is ADHOCw ADA ADwIPCS photon counting acquisition binary int click here for ADA structure ADB ADwT1 global batch macro command ASCII elick here for ADB structure ADC ADw2D context binay internal ADHOC system structure ADH ADwTi Pytheas work Jbinary internal ADHOC system structure ADJ ADw2D ADw8D 16 colors user palette binary internal ADHOC system structure ADL ADwTi general logbook ASCII printable normal ASCII fle ADM ADwT1 macro JAS II oliok here for ADM format ADP ADwTi parameters JASCII lick here for ADP format ADQ ADwT1 parameters spare ASCII click here for ADQ format ADT ADwIPCS acquisition track logbook ASCII click here for ADT format ADV ADw2D crowns parameters ASCII lick here for ADV format ADX ADWT1 photometric correction parameters ASCII click here for ADX format ADZ ADT zones coordinates JASCII lick here for ADZ format ADHOCw HTML help All ADHOCw help is in HTML An internal simple HTML browser is incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file The SWHTML software used is a standalone free shareware The auth
269. ies are RV directly coming from the 2D file 01 projected rotation is PR RV Vs cos 6 Vs where RV is the observed radial velocity Vs is the object systemic velocity is the inclination angle see below p and 6 are the polar coordinates in the plane of the galaxy p and 8 are the polar coordinates in the plane of the sky and 6 are angle with respect to the position angle PA p p and 8 are connected via the following equations tg 9 tan cosi p 6 cos 8 cos 6 Note also the main general basic equation RV Vs Vrot sin i sin 6 Vexp sin j sin Vz cos i where Vexp is the expansion velocity radial in the galactic plane and Vz is the velocity in the direction perpendicular to the galactic plane Quadrants quadrants are numbered 1 2 3 and 4 as graphically shown in the window Possible modes are full image 4 quadrants only quadrant 2 quadrant 3 in position 2 r and V inversed quadrant 4 in position 2 V inversed superposition of quadrants 1 and 3 in position 2 superposition of quadrants 2 and 4 in position 2 Points crowns there are 3 possibilities points are drawn in the same colors than the points of the 2D image as graphs above real colors points are drawn with only 2 colors blue and red corresponding to the different quadrants points are not drawn but crowns are computed The mean value and sigma are computed inside crowns of p The parameter thickness of the
270. ile Reload original profile reloads the original values if they were not already replaced on disk Replace 3D profile in the AD3 file modifies the 3D file 11 Other 3D files remain unchanged The pixels which are modified are all the selected pixels inside the selected cells All these pixels will be put to a unique profile Return quit graph returns to the ADw2D Image folder Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_e htm Return to main ADHOCw menu file C ADHOCw HELP adwa2d_e htm 7 of 8 15 02 02 09 33 54 ADw2D 3D profiles Return to main ADw2D menu file C ADHOCw HELP adw2d_e htm 8 of 8 15 02 02 09 33 54 ADW2D full size of ADw2D_E part 2 M ADHOCw 2D display no ADC context Export display to BMP Setup printer Print Fa Save ADC contest Help X Gui the programy Mouse area 1 Cursor zoom 19x19 pix x it pix Whole image Mouse area 2 Parameters Image p m Action of the left button of the mouse by B epee Er Cros
271. ile names The incemented number integer is indicated by interogative points characters For an integern value a are needed Not used left characters will be set to O Example BES5O1 FlT will indicate files from B5550101 FIT to BSS501 24 FlT Reference slice name 27 Mask file name 3109 3c First channel number p 3 Channels order Channels can be reordered as well as 2D slices file names can be changed In addition itis possible to get automatically the CFHT CURCHAN FITS information for this ordering File suce Hs Modi channels number or a TR z slice file names if needed SLU Cc EL Automatic CFHT ordering Accept the table hal x Abort Bonne for execution cm Iss 3109030 las 109040 Is s10905c eE file C ADHOCw HELP adwft_a2 htm 2 of 4 15 02 02 09 34 07 ADwET slices In order to define the input or output 2D slices 3 steps are necessary 1 to indicate a reference and the total number of channels A reference slice is a file name on which a mask will be put in order to obtain the file names corresponding to each one of the slices If the slice definition is as input give here an existing slice file name If the slice definition is as output give here a typical slice file name this one will not be created as this but will give information to create the set of slice files 2 to indicate the slice mask This mask is built from the reference file name You have just
272. in the VCF driver NOTE the first lines of the DCF or VCF drivers explicit the characteristics of the driver The configuration DEF files contain the information of the acquisition system to use There are some predefined DEF configuration files CHILI DEF for Thomson IPCS 256x256 at ESO GHASP DEF for Thomson IPCS 256x256 at OHP ESO512 DEF for AsGa IPCS 512x512 40 frames s at ESO OHP512 DEF for AsGa IPCS 512x512 40 frames s at OHP QBC512 DEF for AsGa IPCS 512x512 40 frames s at Megantic ESO1024 DEF for AsGa IPCS 1024x1024 20 frames s at ESO OHP1024 DEF for AsGa IPCS 1024x1024 20 frames s at OHP QBC1024 DEF for AsGa IPCS 1024x1024 20 frames s at Megantic But the user can also write his own DEF file and load it A typical DEF file is as following 6000 THT low level 9400 THT medium level 10800 THT maximum 20 Discri file C ADHOCw HELP adwi_a htm 5 of 7 15 02 02 09 34 00 ADwIPCS Parameters 50 TV black level 255 TV white level 0 CS100 interface 0 n COMn 0 shutter system 0 THT system 0 no control 99999v 512 CCD X size 512 CCD Y size 512 stored image X size 512 stored image Y size 40 frames per second 1 ADW3D binning display 0 DALSA high rate swap 1 yes ccir_n dcf Matrox driver for camera vm103_60 vcf Matrox driver for control display END OK button accept the displayed values and go to the acquisition task Abort button
273. inal referential r are given Up to 100 reference pixels can be indicated A least square computation is done in order to get the values of the shifts rotation angle and enlargement factor The ASCII file containing the coordinates to superpose is very simple of the form Xm Ym Xr Yr 1 pixel per line where m represents the coordinates to modify and r the reference coordinates which must be the result It must be 1 pixel per line Comments can be added at the end of the line The number of lines reference pixels is limited to 100 For example 44 3 55 3266 Ist star 38 44 55 second star or 171 294 190 144 star 1 241 445 171 349 star 2 355 340 361 307 star 3 For shifts rotations and enlargement the non existing values are replaced by the substitution value which can be the null value if you load it with the load null into subst button This function can use an execution mask When the execution mask doesn t allow the operation the cube value remains unchanged This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition file C ADHOCw HELP adwt1b11 htm 2 of 4 15 02 02 09 34 43 ADwT1 rotation scaling XYZ translations Example GEOMETRY oper 3 fin Jbx_portable D ADHOCWs_plus BLAISOUS b2_cl ad
274. inates ft 27 E individual sampling Output dimensions Ix ize ly 32 Iz E Founded to lower Execute Heip X Abort Store macro When the user changes the X Y or Z values he lust first reactualize the dimensions a special button appears of data are changed before execution or generation of the macro As the output cube will have different dimensions the output cube will take place in a new directory as well as a new ADP parameter file In this case a special window creating output cubes with different dimensions will appear file C ADHOCw HELP adwt1b10 htm 2 of 5 15 02 02 09 34 31 ADwT1 sub subes or images The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DAS This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example for 3D SUB_ENTITY fin E ADHOCws_plus BLAISOUS lambda ad3 fout E ADHOCws_plus BLAISOUS bidon5 toto ad3 fadp E ADHOCws_plus BLATSOUS bidon5 truc adp nbdim 3 x1 1 x2 256 stepx 2 modex 1 yl 1 y2 128 stepy 4 modey 1 z1 1 z22 27 stepz 2 modez 0 Example for 2D SUB_ENTITY fin E ADHOCws_ plus BLAISOUS somme ad2 fout E ADHOCws_plus BLAISOUS bidon5 toto2 ad2 fadp E ADHOCws_plus BLAISOUS bidon
275. ing analysis 01185 lt 0 22631 1 9544 2 0234453 1 197S 2 5231 3 0 39046 1 2522 2 2568 4 018634 1 028 2 2568 5 096737 0 61387 225231 6 Aa OLA 220081 2485251 7 249201 241298252351 8 24249 370983 2 5231 9 222021 Ae TATT 229089 10 21621 geal 39 2a 2908 1 1 5012 2 0945 2 2369 12 126258 096732 139999 13 122301 141299 2 5231 14 123197 049399 S 1 9544 15 0 99415 0 90125 1 9544 16 123891 04995073 195944 17 12367 1 1005 2 2568 18 1 977 0 87937 1 9544 19 1 3299 1 4477 1 9544 20 1 6429 1 5607 149544 21 1 7335 1 5135 2 9544 22 1 848 1 678 1 5958 23 1 7855 1 7917 1 5958 24 2 0493 1 5763 145958 25 0 95692 1 3959 1 5958 26 0 95078 0 59686 1 5958 27 ADHOCw seeing file dx dy seeing channel Note the presence of a last text line ADHOCw seeing file whatever it contains is necessary to read later correctly the file Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file file CI ADHOCW HELP adwt1_c6 htm 6 of 7 15 02 02 09 34 48 ADwT1 seeing analysis This file is adwt1_
276. io or ellipticity is dedicated to photon counting observations with non solid TV cameras In this case the pixel could be not perfectly square In case of CCD check the X Y forced to 1 check box The user must fill the center of the ring and the X Y pixel ratio if not forced to 1 with approximate values These values will be checked automatically and will see if there is some coherence when computing the phase map At the end of the computation exact values will replace the approximated An error message is given if the center location difference is more than 20 pixels and or the ellipticity difference is more than 10 In case of difficulties you can enforced theses values they will be not changed anyway The including mask is the way to restraint the computation reference to a smaller area By this way you can avoid margin of images Nevertheless the phase map will be computed on the whole field More complex mask refers to executing masks Selective sectors allow to take in account only data of this sector limitation in angles and radii angles are counted anti clockwise from the vertical top line and are in degrees Radii are in pixels center r 0 There are two profile measurement methods slope the parameter nb of channels indicates the number of successive increasing channels in the case of emission or decreasing channels in the case of absorption which determines the edge of the profile The method is the foll
277. ion for the macro command file names is adm Ex MY _ MACRO ADM Execute a macro from an ASCII command file Print instructions PGS SHS nomalzalon OOF CUNT ET SION Var ers a ree Pari EE eng een Anche new_value 4 old_value B ee sua PA Az Edits B Edit About Help X Quit File Translator INSTRUCTIONS FOR THE ADHOCw FILE TRANSLATOR MACRO COMMANDS file C ADHOCw HELP adwft_d htm 1 of 6 15 02 02 09 34 09 ADwET Macros and batch A macro command file is an ASCII file containing macro commands These macro commands are C type commands they may continue on several lines they are always terminated by parameters are separated by space s The default extension for the macro command file names is adm Ex MY_MACRO ADM Each line of a macro is a command a parameter or a comment A Command line begins with FILTRANS and ends with A Parameter line begins with PARAMS and ends with A Comment line begins with and ends with note a space after A macro file log giving the informations on the executed macros is written in the directory containing the macro ASCII command file This log file is named ADW_MAC LOG __PARAMS dd defdir defdir is the default directory If no default directory is mentioned BEFORE a FILTRANS command line fin and fout file names in FILTRANS will be considered to be located in the directo
278. ire de Marseille boulesteix observatoire cnrs mrs fr ADHOCw present version is working on Windows 32 bits systems uses multi tasking and manages completely file sharing on networks Direct dialog or macros can be used There are no size limitations in the 3D dimensions of the data that ADHOCw can reduce ADHOC works mainly on 4 bytes floating values witch offers a large dynamics for the data ADHOCw software is free of use and can be duplicated Information of the interest of users is welcome and a user list is maintained by boulesteix observatoire cnrs mrs fr who will inform regularly of the availability of the new releases Click here to access to the software description Click here to retrieve the last release Click here to return to Observatory home page Since it was created this page was accessed E times file C ADHOCw HELPiindex html 2 of 3 15 02 02 09 33 42 ADHOC software file C ADHOCw HELP index html 3 of 3 15 02 02 09 33 42 ADHOCw software for Windows 32 bits ADHOCw software for Windows 32 bits Interferometry Group Observatoire de Marseille France Version 2001G 21 sep 2001 alyse et LL Li LR ADHOCw A D H O C s What is really new in the last versions General information What is ADHOCw ADHOCw worldwide System and hardware requirements for the Windows version System and hardware requirements for the Linux version Sof
279. irectories In the normal procedure an ADM macro batch file is opened in one single directory and uses a unique ADP parameter file within this directory The user must run again the ADwT1 program to process a data reduction for a different object in another directory With this global procedure successive ADM macro batch files can run successively in different directories The sequence of the commands is located in a ADB global batch file One object one directory one ADM macro file Several objects different directories several ADM files one unique ADB macro batch file A global output logbook file LOG records the successive calls for the ADwT1 program within the different directories It is not possible to run ADwT1 non batch tasks in the same process but note that the user can always run several ADwT1 programs at the same time and so execute normal ADwT1 work even during a global batch process file C ADHOCw HELP adwt1_gf htm 1 of 4 15 02 02 09 34 29 ADwT1 Global macro batch AR ADwT 0 global batch file monitor This monitor allows the user to run bach files successively in different directories In the normal procedure an ADM macro batch file is opened in one single directory and uses a unique ADP parameter file within this directory The user must run again the ADwTT program to process a data reduction for a different object in another directory With this global procedure successive ADM macro batch fi
280. ix C Open a context file ADC previous display parameters X Abort Help i ADHOCw This program can directly read FITS files You can open directly images ADHOC or FITS format or a context file ADC A context file is a special binary file which records the exact parameters of a previous display up to six 2D files and their display levels up to three 3D superimposed files overlays Overlays are texts or drawings lines arrows which are overlayed on the normal displays When quitting the program the following window appears in order to let the user save or not the context into an ADC file file C ADHOCw HELP adwa2d_a htm 1 of 2 15 02 02 09 33 48 ADw2D direct files and ADC contexts ADw2D ADC Do you want to save your work into an ADC context file before quitting The ADC contest files keep the information of the global display different 2D and 3D opened files display levels and colors zoom overlayed text hen running again the ADw2D program and calling the ADE file the et will appear again identical and the different files will be automatically Betun to image No quit immediately Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Net
281. kbox is checked there is a modulo to compute the color and the scale begins again from the bottom when the maximum color is reached To change the step or the threshold there are two ways click on the adequate button or fixed values or edit yourself the step or threshold field Then click on actualize full display Color isophotes color of the isophotes 16 possible basic colors Nb max isoph maximum number of isophotes to be displayed from threshold Avoids to drown pixel subjacent image over a too large number of isophotes Mask file 1 with file 2 values if the user checks this box the values of the image 1 are masked by values of image 2 this means that all the pixels for which the value of file 2 is not inside a given range will not display file 1 null pixels For this a box appears in the top left corner of the window Limits for mask file 2 3 1 E 38 31 E 38 Example of superposition of images The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page file C ADHOCw HELP adwa2d_c htm 3 of 5 15 02 02 09 33 50 ADw2D mixing different displays of images RAMIOCw 20 dinplay nn A y Meat kb Mee ans EO ist im fred ses 4 i Nnc tif th ee F darted ee teete Disian ias E ieoten it maie I Fhrnihdy P Pipbiia
282. kms Profile type Spatial smoothing amp emission C absorption 343 Scale min 180 IV Scale overlap 3 7 Actualize display M OH suppression Interttinge 8 297 Angstroems 378 9 km s smthg 2x2 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_h htm Return to main ADHOCw menu file C ADHOCw HELP adw3d_h htm 3 of 4 15 02 02 09 34 22 ADw3D mono cont RV Return to main ADw3D menu file C ADHOCw HELP adw3d_h htm 4 of 4 15 02 02 09 34 22 Text and overlays ADw2D Return to main ADHOCw help Return to main ADw2D help Text and overlays This function allows to superimpose coordinates texts or drawings on an image 1 Coordinates file C ADHOCw HELP adwa2d_o htm 1 of 6 15 02 02 09 34 23 Text and overlays DO x OR Pate em eA gerd Pe eee X 126 Y 4 M Text coordinates Center Position X 256 00 Y 256 00 C None pixels Screen coordinates 1 to 512 Alpha Delta Crass x Color GE C Arcmin Thick 2 Width 10 Alpha Delta M2 H foo m foco s
283. l is from 402 2757 to 9816 Zoom area button 496 9816 402 2757 6541 291 6570 807 file CI ADHOCW HELP adw2d_zp htm 4 of 7 15 02 02 09 33 56 ADw2D zoom on profiles OI t col OJrU oUr To return to the full spectrum click on the Full spectrum button above the graph To smooth the curve select the smoothing factor could be no smoothing in the box above of the graph A example of the result is shown below ADw2D integrated profile Return to main window Save as ADT hn Smoothing 43 c Eullspectum from 6541 291 to 6570 807 Direct Baycenter Bawcenter cn DE Y from 4022757 lo 496 9816 o vacuus EEE vach To zoom define a rectangle by pres Then press the appearin Free graph label for the user in order to identify or date graphs when printing This label can be edited 496 9816 pee M file C ADHOCw HELP adw2d_zp htm 5 of 7 15 02 02 09 33 56 ADw2D zoom on profiles 402 2757 6541 291 6570 807 To save graph to a BMP file click on the Save as BMP button above of the graph To save graph to a AD1 file click on the Save as AD1 button above of the graph to save in a TXT file which can be edited and displayed by other software s ORIGIN GRAPH_IN_THE_BOX Click here for AD1 format Here the output format will be 2 floating values per line lambda and intensity Example of output AD1 file 6520 000 4
284. l floating pixels DX2 negative DX2 delta x along resulting vertical floating pixels DY2 delta Y along resulting vertical floating pixels F Output 2D eliminated spectra file after coherence elimination Choose file D Pytheas SH1 5ATIGER_eliminated AD 2 file C ADHOCw HELP adwt1_f1 htm 5 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 Output 2D eliminated spectra file after coherence elimination Choose file D Pytheas SH152 TIGER_eliminated AD2 Output 2D remaining spectra file after coherence elimination Choose file D Pytheas SH1524 TIGER_selected AD2 3 Result for next TIGER or PYTHEAS step Output TXT spectra positions file Choose file D Pytheas s H152 TIGER_pos TXT Help X Abort EX Store macro Lens array type presently only hexagonal is working X and Y central position of one of the spectra gives coordinates of the starting micro lens Other position will be computed from this reference position DX1 DX2 DY1 and DY2 give the geometrical parameters of the micro lenses Position of each found spectrum is checked with respect of the reference position and the delta X and delta Y This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example TIGER_POS fcont D Pythea
285. l PA Vs and inclination parameters can be easily obtained by defining very extended crowns in radius for instance 2 symetric crowns with respect to the nucleus or 1 unique covering all the galaxy Note 2 Crown definition r and PA area can be seen when returning to the image and pressing the Edit a paramfr array button ONE crown graph The user can select one to five simultaneous optimizations Xc center position Yc center position position angle of the major axis systemic velocity galactic plane inclination To better optimize the Xc and Yc position it is possible to symetrize radii click checkbox This means that all the positive radii will be folded to negative radii In this file C ADHOCw HELP adw2d_k2 htm 9 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns case the sigma of the rotational velocities is compute with points appearing at the same crown radius range but in opposite sectors Note that for Xc and Yc variations only the computation of the rotation velocity is affected the selected sectors remain unchanged This means that there are two centers one for the rotation curve one for the defined geometrical sectors The computation time varies as the number of iterations The computation time can be huge if the number of iterations is important We recommend to the user to begin with a small number of iterations The principle of this optimization is
286. le browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b8 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b8 htm 4 of 4 15 02 02 09 34 40 ADwT1 figure BO8 full size ADw smoothing ADHOCw JO special smaathing m User smoothing can select and edit defined smoothing store and load user matrix file C ADHOCw HELP AdwT 1 B8t htm 15 02 02 09 34 41 ADwT1 spatial smoothing ADwT1 Return to main ADHOCw help Return to main ADwT1 help B09 Spatial smoothing for 2D or 3D files The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for helo manual on paper see next page file C ADHOCw HELP adwt1_b9 htm 1 of 6 15 02 02 09 34 42 ADwT1 spatial smoothing ADHOCw xa 2 D 8 UN D 0 amp BR D D om ln or JO spste scott 3 ance D k Choose fle Mok OO O OO OO Ou a ma mk D L 1 D 1 D L l D L l D 1 L Jup al cri fie ihana tal naal iniy fille Tn ee O OO 0 0 0 M 0 Hore cithe ior A opt gute de enc lo DIE IL DATE CETTE RTS
287. les can run sucessively in different directories The sequence of the commands is located in a ADB global batch file One object one directory one ADM macro file Several objects different directories several ADM files one unique ADB macro batch file global output logbook file LOG records the successive calls for the ADwT1 program within the different directories It is not possible to run ADwTT non batch tasks in the same process but note that the user can always run several ADwI1 programs at the same time and so execute normal ADwT1 work even during a global batch process Be E AD ADwTO ADB editor ADHOCw ADwT1 global macro batch editor Directory path ADP parameter file ADM macro file 1 D Data annie s642 TITLADP bidon adm 2 D autre _repertoire autre_ sous_repertoireencore encore2 C345 ADP C345 ADM 3 c data 342 4DP macro adm 7 file C ADHOCw HELP adwt1_gf htm 2 of 4 15 02 02 09 34 29 ADwT1 Global macro batch lt PRESPREERPEEEPEEEEREEDI ADB command file structure It an ASCII file Each line contains 3 strings executing path ADP parameter file ADM macro file file C ADHOCw HELP adwt1_gf htm 3 of 4 15 02 02 09 34 29 ADwT1 Global macro batch Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHO
288. lorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_a2 htm Return to main ADHOCw menu Return to main ADWFT menu file C ADHOCw HELP adwft_a2 htm 4 of 4 15 02 02 09 34 07 ADwET 2D and 3D translations Return to main ADHOCw help Return to main ADWFT help ADwFT 2D or 3D simple translations To translate simply a 2D image or a 3D cube into a different format click on the 2D gt 2D folder or the 3D gt 3D folder select the input and output formats and execute 3D input and output accepted formats AD3 floats 32 ordered by spectra default DA3 integers 16 ordered by spectra new ordered by channels floats 32 ordered by spectra floats 32 ordered by channels floats 32 ordered by channels uncommon 16 ordered by spectra ordered by spectra 16 ordered by channels loats 32 ordered by channels 16 ordered by spectra ordered by spectra 16 ordered by channels ordered by channels floats 64 ordered by spectra floats 64 ordered by channels ADHOCw PC ADHOC old ELC compressed FITS 3D FIT FITS 3D FIT ADHOCw PC AD3 Binary or IDL PC integers Binary or IDL PC floats 32 Binary or IDL PC integers Binary or IDL PC f Binary or IDL Unix integers Binary or IDL Unix float
289. lp adhocw htm file This file is adwt1_b3 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b3 htm 3 of 3 15 02 02 09 34 38 ADwT1 maximum and minimum ADwT1 Return to main ADHOCw help Return to main ADwT1 help B04 Minimum and maximum of a file ADHOCw Atinimumcmenimum af a ZOID fle Input 2D or 3D file Use an execution mask Execute 7 Help x Abort EX Store macro This program computes the minimum and maximum of files It accepts 2D or 3D files it recognizes automatically the type of the input file The input file is not modified The null values are not taken in account The input null values are not taken in account in this computation The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output information gives the X Y Z coordinates of the minimum and maximum Coordinates are numbered from 1 This function can use an execution mask file C ADHOCw HELP adwt1_b4 htm 1 of 3 15 02 02 09 34 38 ADwT1 maximum and minimum This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example MINMAX fin D ADHOCws_plus BLAISOUS Call da3
290. ls The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD2 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network file C ADHOCw HELP adwt1_b1 htm 1 of 3 15 02 02 09 34 37 ADwT1 sum of the channels Macro definition Example SUM3D2D fin D ADHOCws_plus BLAISOUS Oba da3 fout D ADHOCws_plus BLAISOUS sum_oba ad2 keyword content options sumoa Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b1 htm file C ADHOCw HELP adwt1_b1 htm 2 of 3 15 02 02 09 34 37 ADwT 1 sum of the channels Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_b1 htm 3 of 3 15 02 02 09
291. ly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_tp htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_tp htm 3 of 3 15 02 02 09 34 33 ADwT1 TIGER 1 ADwT1 Return to main ADHOCw help Return to main ADwT1 help F01 TIGER spectra position extraction from continuum image How to reduce TIGER Function F01 This function is the first step for TIGER and PYTHEAS data reductions This function recognize spectra from continuum and tabulates their positions Procedure 1 the program searches individual continuum spectra 2 it selects them from width and length 3 selects additionally from the geometry 4 it builds a TXT editable position file to enter in the F02 function To check after execution nb of remaining final spectra log information selected and eliminated spectra in special 2D files file C ADHOCw HELP adwt1_f1 htm 1 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 ADHOCw F01 FIGERPITHEAS spectra position extraction fram continuum mage 1 Extraction parameters Input 2D continuum file D Pytheas SH152 sum_P040_ad2 Output 2D verification spectra file extraction only Choose file D Pytheas SH152 TIGER_extracted AD2 2D input file intensity thr
292. ly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example CORREL_ OH fin E ADHOCws_plus BLAISOUS Oba da3 ph_prb E ADHOCws_plus BLATSOUS Phas_prb AD2 fzones E ADHOCws_plus BLAISOUS Zones adz fphotom E ADHOCws_plus BLATSOUS bidon adx mode_ref 0 control_bmp 0 beam 5 bkgd 0 15 phase_corr 0 ke yword content options CORREL_OH OH f es input not dephased file name with in whole path p h_prb 2D parabolic phase with whole path fzones ADZ input file containing selected areas fphotom ADX output file to store photometric coefficients mode_ref mode of 2D reference file 0 no file 1 file indicated in fref fref 2D photometric reference file if mode_ref 1 control_ bmp mode for the BMP control files 0 no control 1 BMP files will be stored beam pixel beam for example 5 is 5x5 pixels file C ADHOCw HELP adwt1_c5 htm 6 of 11 15 02 02 09 34 46 ADwT1 photometry from OH bkgd background noise cut noise background noise eut phase corr micro phase correction NO A yes Log book results Excepted the text of the macro and the ending execution message the following information is recorded
293. lyzing channel 18 0181 01 Lower 2 08 19 a 0 826222 b 0 500858 0181 01 Lower 2 08 19 Analyzing channel 19 0181 01 Lower 2 08 20 a 0 954282 b 7 099259 0181 01 Lower 2 08 20 Analyzing channel 20 0181 01 Lower 2 08 21 a 0 864779 b 4 638884 0181 01 Lower 2 08 21 Analyzing channel 21 0181 01 Lower 2 08 21 a 0 782870 b 6 735388 0181 01 Lower 2 08 21 Analyzing channel 22 0181 01 Lower 2 08 22 a 0 809161 b 5 007386 ADwT1 photometry from OH Expected results 0181 01 Lower 2 08 22 Analyzing channel 23 0181 01 Lower 2 08 22 a 0 912076 b 5 600414 0181 01 Lower 2 08 22 Analyzing channel 24 0181 01 Lower 2 08 23 a 0 830078 b 1 183846 0181 01 Lower 2 08 23 Analyzing channel 25 0181 01 Lower 2 08 23 a 0 904278 b 8 330544 0181 01 Lower 2 08 23 Analyzing channel 26 0181 01 Lower 2 08 24 a 0 776713 b 8 285838 0181 01 Lower 2 08 24 Analyzing channel 27 0181 01 Lower 2 08 25 a 0 808451 b 9 512576 Suppose that you look to a normal CCD CFHT observation The analysis with this function will give an ADX file which is for instance A and B for Y AX B 1 49872 38 011 channel 1 1 09942 5 81679 channel 2 1 1452
294. m must be near 100 If not this means that the computer is overloaded and cannot run all the simultaneous tasks with efficiency Photons can be lost THT intensifier file C ADHOCw HELP adwi_d htm 2 of 4 15 02 02 09 34 03 ADwIPCS acquisition tune THT THT tuning window appears The user can change the THT manually emergency stop the THT downs immediately to OV Shutter open opens the shutter close closes the shutter automatic the shutter automatically closes if the photon rate exceeds a given value which is a strong protection to high accidental illuminations In any case if the shutter is closed a warning appears for the user TV parameters allow modification wakes up this function which is not usually enabled It is suggested not to change the TV parameters during the observation Anyway the modification is very slow and the user must wait some seconds before any effect R4 stores 4 successive frames to check the remanence The frames are put in the C root directory Acquisition buttons Start at beginning or after suspension Suspend after beginning The acquisition is frozen A dialog proposes to start again at one channel chosen by the user Abort and Quit This window always stays in front If exceptionally the user wants to let the possibility to load in front of the screen another program he can allow this By default the acquisition window is always in
295. m the seeing transparency and background effects along the exposure For IPCS many scans are integrated along the exposure typically one elementary image is 10 seconds so for 24 channels the scanning time is 4 mn Then all the scans are added in order to build one unique cube In this case the seeing and transparency conditions are perfectly averaged this is not the case for CCDs for which the read out time and specially the necessity to have minimum exposures of some minutes in order to minimize the read out noise and to reach better sensitivity reduces usually the number of scans to 1 The correction of the seeing transparency and background effects is in this case extremely important Some observational methods interlaced scans can decrease these effects but a rigorous correction is always needed In fact for CCDs 3 additional corrections are necessary the cosmic rays correction eventually the seeing and displacement correction the transparency and sky background corrections 1 Getting the data cubes At minimum two cubes are necessary to reduce CIGALE data 1 object cube and 1 calibration cube The best is to have on calibration before the observation and one after in order to check the correct functioning of the interferometer There are different cases depending of the origin of the data 2 Running the ADwT1 program file C ADHOCw HELP adw_proc htm 1 of 5 15 02 02 09 34 47 ADHOCyw
296. m x 2 centered at the mouse location Similarly you can unzoom of a factor 2 by clicking on the right button of the mouse but pressing at the same time the shift key Another way is to change the Image area box which gives the size of the displayed image Graph area change this to display all the channels at the same time Field You can move the field by changing the X0 and YO values Palette You can change the color palette different rainbows black and white color inversions user palette User palette allows the user to define himself the colors Step threshold and scale overlap The correspondence between the values of the image and the colors is obtained from 3 parameters the threshold lowest displayed value the step space between colors and the possible overlap If there is no scale overlap all the values larger than the last step are displayed like the last step If the scale overlap checkbox is checked there is a modulo to compute the color and the scale begins again from the bottom when the maximum color is reached To change the step or the threshold there are two ways click on the adequate button or fixed values or edit yourself the step or threshold field Then click on actualize full display Zoom area pixel and channel position value On the top of the screen the left image usually represents the 19x19 pixel zoom of the mouse position On the right the values of the XYZ position and the conte
297. measured spectra log information 2D calibration verification file ADw2D with on line measurement of the wavelength on the profiles F02 ADw TIGER creation of wavelength cube p Dj x file C ADHOCw HELP adwt1_f2 htm 1 of 8 15 02 02 09 34 33 ADwT1 TIGER 2 ADHOCw TIGER creation of the JO wavelength cube Input TXT spectra positions file from function FOT Choose file D Pytheas sh1 52_jlg TIGER_pos TXT Spectrum extension to gt left to detect calibration lines pixels Input 20 observation file Choose file D Pytheas sh152_jlg somme_P038_sans_bias_sans_cosmiques ad2 Spectrum extension to gt right to detect calibration lines pixels 1 Calibration parameters Input 20 calibration lines file Choose file D Pytheas sh152_jlg somme_P033 ad2 i T n me E ad O 1pix 2 5pix Sense of wavelength from left to right 2D input file intensity threshold to separate the lines Height of measure for one spectrum pixels increasing gt 6506 528 6532 882 6598 953 Calibration wavelengths increasing wavelengths in Angstroems Load array from TXT file Save array into TXT file Polynomial degree of the interpolating wavelength dispersion curve polynomial 1 line 2 parabola ie Output 20 verification spectra file lines position file C ADHOCw HELP adwt1_f2 htm 2 of 8 15 02 02 09 34 33 Choose file 3 Geometrical output sampling
298. menu The user must first define the output directory which must be different of the current one This directory can be simply opened if it exists or created Then the user defines the output data file name and the output name Then he can return to the calling function menu return to the previous menu For example the windows becomes the following if the user wants to open an already file C ADHOCw HELP adwT1oth htm 2 of 4 15 02 02 09 34 30 ADwT1 Other ADP directory existing directory ADHOCW New output diectory The dimensions of the output file will be different from the current parameters You cannot in this case create the output file in the current directory You must define or create a new directory where the output file will be created and where a new parameter file will be also written with ne new dimensions EADHOCWs_plus BLAISOUS Choose one existing directory and press Open this directory ADHOCws_plus Open this directory BLAISOUS Comment or information file C ADHOCw HELP adwT1oth htm 3 of 4 15 02 02 09 34 30 ADwT1 Other ADP directory boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings
299. meters the Signal to Noise is here If not you can loose easily a factor 2 in detection AD ADHOCw Test grabing photon counting Wrarning You need an auxiliary TY monitor connected to the VGA plug of the MATROX board for these tests Test MATROX and centroiding with auxiliary TV display tf TY IPCS Random simulation Discri i l Black iul 135 aid White lul 150 Ea def 20 see def 51 def 255 E relief unusual _Tune THT Test PerotFabry with auxiliary TV display QGcst 3210 Imbd 6562 78 nhc 24 FFetep 29 690 Ffbasez 3596 206 E5700 serial interface CUMA H channel FF value 100 E Move PE file C ADHOCw HELP adwi_e htm 3 of 4 15 02 02 09 34 04 ADwIPCS tuning youuu es Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwi e htm Return to main ADHOCw menu Return to main ADWIPCS menu file CI ADHOCW HELP adwi_e htm 4 of 4 15 02 02 09 34 04 ADw3D_IPCS ADw3D Return to main ADHOCw help Return to main ADWIPCS help ADW3D display as slave program o
300. n F01 TIGER spectra position extraction from continuum image F02 TIGER creation of the 3D wavelength cube gt Edit a batch file SZ Exec a batch file Show logbook Ex Display control Help Quit the program Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the _ADL ascii log file which contains the sum of all the log books of the successive sessions For that press the Show logbook button above at any time file C ADHOCw HELP adwt1_f htm 1 of 2 15 02 02 09 34 56 ADwT1 menu TIGER F01 TIGER spectra position extraction from continuum image F02 TIGER creation of the 3D wavelength cube Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_f htm Return to main ADHOCw menu Return to main ADwT1 menu file CI ADHOCW HELP adwt1_f htm 2 of 2 15 02 02 09 34 56 ADwT1 menu PYTHEAS ADwT1 Return to main ADH
301. n deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation ADwT1 PYTHEAS 1 0182 16 Batch Lower 18 16 28 G01 1 444 channels 0182 16 Batch Lower 18 16 28 G01 1 767 channels 0182 16 Batch Lower 18 16 28 G01 2 091 channels 0182 16 Batch Lower 18 16 28 G01 2 415 channels 0182 16 Batch Lower 18 16 28 G01 2 737 channels 0182 16 Batch Lower 18 16 28 G01 3 062 channels 0182 16 Batch Lower 18 16 28 G01 3 385 channels 0182 16 Batch Lower 18 16 28 G01 3 709 channels 0182 16 Batch Lower 18 16 28 G01 4 033 channels 0182 16 Batch Lower 18 16 28 G01 4 356 channels 0182 16 Batch Lower 18 16 28 G01 4 680 channels 0182 16 Batch Lower 18 16 28 G01 5 004 channels 0182 16 Batch Lower 18 16 28 G01 5 327 channels 0182 16 Batch Lower 18 16 28 G01 5 651 channels 0182 16 Batch Lower 18 16 28 G01 5 975 channels 0182 16 Batch Lower 18 16 28 G01 6 298 channels 0182 16 Batch Lower 18 16 28 G01 6 621 channels 0182 16 Batch Lower 18 16 28 G01 6 945 channels 0182 16 Batch Lower 18 16 28 G01 7 270 channels 0182 16 Batch Lower 18 16 28 G01 7 592 channels 0182 16 Batch Lower 18 16 28 G01 7 916 channels 0182 16 Batch Lower 18 16 28 G01 PYTHEAS_ CUBE Info PYTHEAS_ CUBE Info PYTHEAS_
302. n 1 08544 3 47297 chann 1 29321 10 4741 chan 141239 9 61532 Iehann 1 21228 2 67023 chan 0 987761 9 15051 cha L16882 7 525232 chan L20114 2 72319 Iehan 1 23074 7 10736 chan 1 10415 8 04011 chan 1 02561 5 41701 chann 1128587 15 8557 leban 1 00803 0 12065 chann 1 192978 1 28688 chan 1 13325 2 65948 chan 1 17313 10 0865 lchan 1 21033 0 606203 leha el 1 A and B for Y AX B el 2 A and B for Y AX B l 3 A and B for Y AX B el 4 A and B for Y AX B 1 5 A and B for Y AX B el 6 A and B for Y AX B nel 7 A and B for Y AX B el 8 A and B for Y AX B el 9 A and B for Y AX B el 10 A and B for Y AX B el 11 A and B for Y AX B 12 A and B for Y AX B el 13 A and B for Y AX B 14 A and B for Y AX B el 15 A and B for Y AX B 6 A and B for Y AX B A and B for Y AX B nel 18 A and B for Y AX B 0 0 J 2 SB og SNS 5 O Sie D Se SES a O SS O 5 i i L 1 04791 7 43938 channel 19 A and B for Y AX B 1 15636 5 36424 channel 20 A and B for Y AX B 1 27735 8 60345 channel 21 A and B for Y AX B 1 23585 6 18837 channel 22 A and B for Y AX B 1 0964 6 14029 channel 23 A and B for Y AX B 1 20471 1 42619 channel 24 A and B for Y AX B 1 10585 9 21237 channel 25 A and B for Y AX B 1 28748 10 6678 channel 26 A and B for Y AX B
303. n 4000 00 _Save graph to BMP PE OM 1938 ET50FS 1034 MARSEILLE 5 Lambda max 7250 00 X Quit gt Finesse min 0 00 Choose an talon and excute Finesse max 90 00 a This graph displays THOERETICAL Finesse and spectral resolution for a point pupil For a full pupil 30 to 45 mm divide these values approximately by a factor 2 Finesse a PF OM 1938 ETSOFS 1034 MARSEILLE 5 p 1938 656278 4 Transmission 100 CURRENT MOUSE wavelength 4 80 eee ESEE FEE EN ee Ni ere MR doses ete couide Lab EEE EE EEE file CI ADHOCw HELP adwti_h9 htm 1 of 3 15 02 02 09 35 03 5752 0 transmission 3 8 reflectivity 2 96 2 Finesse ADwT1 Perot Fabry talons 50 interf order 2211 delta lamdba 4 2 602 delta lambda km s 135 55 spectral resolution 179015 resolution 4 0 032 resolution km s 1 67 The user can select an interferometers from a list and draw the transmission and Finesse curves The user can modify the drawing limits and scales Moving the mouse inside the graph allows to get current values of the interferometer at the given wavelength When pressing the Show QG constants the user has access to an array of scanning constants for different etalons and CS100 controllers E H09b ADw Queensgate constants BE x ADHOCw Queensgate constante WAE Nr Let know eventual changes to boulesteix observatoire_cnrs mrs fr in order to u
304. n order to be informed of the new releases and of the solution of problems JBx 19 02 99 After installation the following files must be present 1 Directory ADHOCW ADHOCW EXE ADW2D EXE ADW3D EXE ADWFT EXE ADWT1 EXE ADWIPCS EXE only for photon counting Matrox acquisition CCIR_N DCF if ADWIPCS EXE is present AXDRV IN if ADWIPCS EXE is present CHILI DEF if ADWIPCS EXE is present GHASP DEF if ADWIPCS EXE is present 2 Directory ADHOCW HELP numerous HTM files numerous GIF files some JPG files HACCESS CTL SWHTML EXE L B31HT DLL ADHOCMAN DOC Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_inst htm Return to main ADHOCw menu file C ADHOCw HELP adw_inst htm 2 of 3 15 02 02 09 35 06 ADHOC software installation file C ADHOCw HELP adw_inst htm 3 of 3 15 02 02 09 35 06 ADHOCw
305. n the TV control display and adjust the THT value with the observation brightness The risk is maximum Discri is the binarization level for the Matrox board This value must be tuned and set with the Test Matrox function TV black level is needed for the Matrox board This value must be tuned and set with the Test Matrox function TV white level is needed for the Matrox board This value must be tuned and set with the Test Matrox function CS100 interface is the manner to drive the Queensgate Controller It could be parallel or serial For ESO it is 0 parallel interface For OHP it is 2 COM2 serial interface If there is no CS100 the user can put here a dummy value and then indicate on the menu that the scanning is not performed Shutter system can be O no shutter 1 OHP 2 Chili 3 AsGa or more depending of the further systems THT system can be 0 no THT system 1 OHP 2 Chili 8 AsGa or more depending of the further systems CCD X size is the physical horizontal CCD size to read It is 768 for Thomson and 512 or 1024 for DALSA AsGa depending if there is or not an hardware binning CCD Y size is the physical vertical CCD size to read It is 288 for Thomson and 512 or 1024 for DALSA AsGa depending if there is or not an hardware binning Stored image X size is the size of the recorded photons X addresses For DALSA AsGa it is usually the same value that CCD X size there is no interest to decr
306. n this case a photometrical correction is done This option is strongly recommended Correct from remanence is an option that doesn t integrate the photons of a given frame if another photon was present at the same location in the previous frame You can define the location where the pixel is supposed to be remnant same pixel 3w3 pixels 5x5 pixels or 7x7 pixels Be careful if the flux is high this option can allow the program to ignore successive photons even if most of them are not remnant This option is not suggested for calibrations Suppress external TV parasites is an option which allows to suppress frames with abnormal counting rates You can decide of the acceptable sigma All the frames which have a counting rate larger than the mean value this acceptable sigma will be suppressed and not counted The result will be ponderated i e the fact that the frame is missing will be taken in account if the Normalize exposure from frame count option is active You can integrate successive cycle as you wish by choosing the beginning and ending integration cycles in the Integrate cycle section Memory needed in order to increase the speed of the integration the program creates in memory a global cube The request memory is therefore large Counting statistics these statistics are written in the log book For one frame you get for example 0003 01 Lower 18 31 10 moy sig discri 8 9 5 6 37 0003 01 Lower 18 31 10 fr
307. n to main ADwT1 menu file C ADHOCw HELP adwt1_g htm 2 of 2 15 02 02 09 34 57 ADwT1 menu MISCELLANEOUS ADwT1 Return to main ADHOCw help Return to main ADwT1 help Miscellaneous functions H 2 ADwT1 W005 OF x Hide task manager window Sia ARSE Rane A D H O Cw A DwT1 Version 2000L JBx Obs Marseille 1280 s 1024 96 ppi General 2D 3D operations Cigale Profiles IPCS Tiger Pytheas Miscell Dummy operation for tests of the ADwT1 task nucleus Translation of a parabolic phase into an old ADHOC DOS phase Creation of a dummy homogeneous 2D or 3D file 4 Instrument tuning using image sequences Various peculiar cube corrections F Exec a batch file Precessions and object visibility _ Sideral time clock Edit a batch file LSJ Interference filters selection a Perot Fabry talons characteristics and Queensgate constants Est Display control Common nebular and calibration wavelenths Quit the program 7 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions H01 function Dummy operation for tests of the ADwT1 task nucleus file C ADHOCw HELP adwt1_h htm 1 of 2 15 02 02 09 34 58 ADwT1 menu
308. nd other Intel AMD or Cyrix equivalent chips Executable code is optimized for speed execution 16 Mb memory for Windows 95 98 and 32 Mb memory for Windows NT 2000 is a minimum 32 48 Mb and 64 96 Mb are respectively recommended Tiny memory increases the frequency of swaps on disk and therefore reduces the execution speed of the programs 1024 x 768 x 256 screen is recommended for 2D display 1280 x 1024 x 256 screen is recommended for 3D display Nevertheless the software runs always with reduced screen dimensions The recommended screen parameters for the different ADHOCw programs are program screen size nb of colors pixels per inch ADw2D 2D display program 1024x768 256 96 ADw3D 3D display program 1280x1024 256 96 ADwT1 data reduction program 800x600 16 96 ADwFT file translation program 640x480 16 96 ADwIPCS photon counting acquisition program 1280x1024 256 96 Printers available inside Windows are used by ADHOCw but Window print screen programs Pizzazp Printscreen are recommended One of these tools is available on the ADHOCw Internet access http Awww obs cnrs mrs fr System and hardware requirements for the Linux version The ADHOC ADHOC for Linux version will be available at the end of the year 2001 file C ADHOCw HELP adw_what htm 2 of 15 15 02 02 09 33 45 ADw what is ADHOCw Running ADHOCw The main program dispatche
309. nd the coordinates are rearranged in order to have x2 gt x1 and y2 gt y1 but the original file is not changed The ADZ zones file is compatible with the old ADHOC DOS area files functions 13 and 48 The only change is that the coordinates can be now float and not limited to integers 0 or 999 values are not taken in account as well that comment lines at the end For instance the following file which is coming from an old ADHOC sequence is valid 35 23 245 101 Zone 1 280 353 532 475 Zone 2 4 175 500 207 Zone 5 5 249 302 351 Zone 7 143 313 241 389 Zone 9 143 453 143 453 Zone 11 0 0 0 Zone 3 O 0 Zone 4 0 Zone 6 0 Zone 8 0 Zone 10 999 999 999 Zone Q oO 0 0 0 0 O O O O file C ADHOCw HELP adwt1c11 htm 2 of 8 15 02 02 09 34 53 ADwT1 rough photometry zones Possible input for numerous ADHOC functions but new files as the following are also valid 171 5 294 78 190 144 area 1 241 445 171 2 349 0 area 2 355 340 361 307 area 3 999 0 0 0 area 4 999 0 0 0 area 5 999 0 0 0 area 6 999 0 0 0 area 7 999 0 0 0 area 8 999 0 0 0 area 9 999 0 0 0 area 10 999 0 0 0 area 1 zones Possible input for numerous ADHOC functions The output ADX ASCII file is a file which will be used further for the photometric correction It has the following structure 1 01887 13 9705 ehan LALSSESTL 7 95 7 594 cha
310. new ADHOCw type AD3 or old ADHOC type DA3 When the user press on the Execute button the Finesse is computed and its drawing appears file C ADHOCw HELP adwt1_c9 htm 2 of 5 15 02 02 09 34 52 ADwT1 Finesse ADHOCW Ainesse of the calibration Input 3B file calibration Choose file E ADHOCws_plus BLAISOUS Cal1 da3 Input 2D parabolic phase Choose file E ADHOCws_plus BLAISOUS Phas_prb AD2 Zone of integration 1192 1 192 to k2 320 21320 uel _X avort ne _ ue x a be run in neh Finesse 9 56 Save profile to ADM Print the graph Input calibration tle Call das Input phase file Phas_prb AD Zone 192 192 to 320 320 16641 psels Computed Finesse 9 66 Save graph into BMP Quit this function Save profile to AD1 saves the profile values to an AD1 file Click here for AD1 format Print the graph prints the window Save the graph into BMP saves the graph area into a BMP image file Quit this function returns to main ADwT1 menu file C ADHOCw HELP adwt1_c9 htm 3 of 5 15 02 02 09 34 52 ADwT1 Finesse Example of AD1 file output 2 387E 0 1 729E 0 1 373E 0 1 159E 0 L 018E 0 9 204E 0 8 505E 0 8 7 DS D OO I I I WI a 012E 0 666E 06 7 431E 0 7 313E 0 7 3E 0 408E 0 663E 0 119E 0 844E 0 9 94E 0 1 165E 0 19 1 44E 0 20 1 901E 0 21 2 765E 0 22 4 746E 0 23 9 677E 0 24 1 66E 0 25 1 514E 0 26 7 655E 0 27 3 835E 0
311. ng the observation the user can modify the THT value by pressing on the Tune THT buttons that appear in different windows All these buttons have the same effect Note that the user can always disable the THT direct tuning for example to tune the THT manually For that simply edit the C ADA DEF ASCII file which contains the running parameters and set the THT system parameter to 0 When pressing the Tune THT button the following window appears LE ADHOCw tuming THT Biel x ADHOCw Photon Counting THT 010101010 volts Down to 6000n Up to 840i Down to S40 Up to masimum 10600 ine mantally up te maximum Stop positionning Down to 0 V Track cursor to change THT Click inside the white tackbar to change only a step of 1 Volt Return to acquisition file C ADHOCw HELP adwi_c htm 1 of 3 15 02 02 09 34 02 ADwIPCS THT a KEWU to acquismion The THT can be tuned by steps As the speed of the THT increasing is extremely important for the repetability of the enlargement scale pixel of the electrostatically focused integration tubes the program increases first the THT regularly First stage is up to 6000V this value is defined in the GHASP DEF CHILI DEF and C ADA DEF ASCII files during this step there is in principle no danger even dome illumination has no effect because the intensification is low Second stage is up to 9400V this value is defined in the GHASP DEF CHI
312. ng value to hull value fF Execute Help x Abort This program creates a 2D or 3D file which will be filled with a constant value This function is interesting in order to create execution masks from nothing and edit them with the_ ADw2D program Store Macro The user must only give the name of the 2D or 3D output The output file is created as new file C ADHOCw HELP adwt1_h3 htm 1 of 3 15 02 02 09 34 58 ADwT1 creation a dummy homogeneous file ADHOCw type AD2 or AD3 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example FILI DUMMY fout E ADHOCws_plus BLAISOUS bidon ad3 nbdim 3 value 3 1E 38 keyword content options FIL DUMMY Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information file C ADHOCw HELP adwt1_h3 htm 2 of 3 15 02 02 09 34 58 ADwT1 creation a dummy homogeneous file boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction
313. ng values are accepted The center coordinates are ADw2D compatible numbered from 1 Systemic velocity this is the real velocity of the center coherent with the radial velocities values contained in the 2D file 01 Rotation velocities radial velocities projected rotation the user must choose here what to draw rotation velocities are Vrot p RV Vs sin cos 6 radial velocities are RV directly coming from the 2D file 01 projected rotation is PR RV Vs cos 6 Vs where RV is the observed radial velocity Vs is the object systemic velocity is the inclination angle see below p and 6 are the polar coordinates in the plane of the galaxy p and 8 are the polar coordinates in the plane of the sky and 6 are angle with respect to the position angle PA p 0 p and 6 are connected via the following equations tg 9 tan 0 cos i p 0 cos 0 cos Note also the main general basic equation RV Vs Vrot sin ji sin 6 Vexp sin i sin 0 Vz cosi where Vexp is the expansion velocity radial in the galactic plane and Vz is the velocity in the direction perpendicular to the galactic plane Inclination with respect to sky plane this inclination angle given here in degrees is 0 if the galaxy is face on and 90 if the galaxy is edge on Position angle with respect to bottom top this position angle given here in degrees is 0 if the PA points to the top of the 2D image 90 if the PA points
314. ngs The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwtic10 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1c10 htm 4 of 4 15 02 02 09 34 30 ADwT1 sub subes or images ADwT1 Return to main ADHOCw help Return to main ADwT1 help B10 Extraction of a sub cube 3D or a sub image 2D This function allows to create new cubes or images extracted from existing cubes or images and therefore of different dimensions Bounding coordinates are not excluded The user can indicate a step and choose between binning integrate the values located inside the step or individual sampling only one pixel is taken to sample the image or the cube This choice has no meaning if the step is equal to 1 In the case of binning if one of the value is a null value this value is not taken in account in the integration If no binning occurs the null values are always taken in account file C ADHOCw HELP adwt1b10 htm 1 of 5 15 02 02 09 34 31 ADwT1 sub subes or images po ADw sub cubes or images ADHOCw Extraction OF G SUD CUBRE 90 er amp sui ages Ci sub cube 30 extraction sub image 20 extraction Input 30 file Output 300 file Choose file Outut ADP parameter file defined with the output 3D file Neva Oo from step to coordinates i 256 2 binning Y coordinates fi i 28 4 binning Z coord
315. nimum and maximum values You can also draw X or Y grids with the spacing you wish Another possibility is to print or save on disk the cross section values file C ADHOCw HELP adwa2d_d htm 1 of 3 15 02 02 09 33 52 ADw2D cross sections Thick cross sections simply edit the thickness value box The following image illustrates a thick cross section on a dual visualization Square pixels and isophotes The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens to visualize the figure with full resolution for help manual on paper see next page LEE w 1522 RE im ME vn CA Cipot digio IMT 2S eue peer Pt PI y E Se dit corte fi Kred x it the pound 5 5 Meer cam Live Marc gra von DEM tee TT ot ie BS Pivteds ome mir K petro Jee OCT vi ee went mage m1 Li Parad Tee TS Led lies of Ther em ener image Ni fn dr bated je eteate Ping deg memmen P a 4 p d O idy M Fpl r lavey iras Di atk po d ki Time sms Fes f 5 Marton r Iny n at innn ju PTS 0 METS ates _ Mine TAMIL UN VUN i pt 4 3 y 0 Laeet cade ree ELITE 1 J r iM ae QI 2l MATE in Yh Ss sl at Tai i ww 4 Pe anh gt 3 My cies k J 108 1000 FA i Virusles en nsis AURAS LES aa bi Gaus set r2 ij 7 VAUT r Jie saline saf heruptse K ping Comment or information
316. normal the lens is suppressed Number of the most intense line if there are many calibration lines it is possible to avoid elimination from the sigma as above if there is a mistake on the sequence of the lines for example a faint first line missing The program can take as reference calibration line the most intense If this value is 0 this procedure is not used 3 Geometrical output sampling parameters This are the parameters defining the output cube The L D and alpha angle sampling values are defined as in the upper figure The define the output image sampling L is only used in order to find the 3 nearest lenses for a sampled pixel Use ADw2D on calibration 2D file to compute it Compute on 10 lenses As L is only used to reject distant lenses L could be approximated to a pixel Dis used to define the output sampling Note that D lt L sqrt 3 2 is udersampled The alpha angle is used for the orientation of the output image with the north for instance Automatic origin if not checked the center of the image is taken If checked an arbitrary position can be chosen The D increment if done from this reference position Starting wavelength ending wavelength and step define the wavelength sampling 4 Reference zero wavelength This value is set in the new ADP file in order to compute velocities from the wavelength cube It is the zero wavelength of the object 5 Result file C ADHOCw HELP adwt1_f2 htm 4 of
317. nown open unit 22 file float idl access direct recl Iz 4 status unknown c array initialization do 1 k 1 Iz itab k k tab k k 1 continue c writing the 3D data profile do 11 j 1 ly do 11 i 1 Ix index j 1 Ix write 21 rec index itab k k 1 1z write 22 rec index tab k k 1 1z 11 continue c closing files close 21 close 22 end Example of program in C for 2D images and integers 2 and floats 4 int Ix 50 ly 60 i j float tab short int itab tab new float Ix itab new short int Ix opening output files lu_int sopen int idl O_BINARY O_ RDONLY SH_DENYNONE lu_float sopen int float O_BINARY O RDONLY SH DENYNONE array initialization file C ADHOCw HELP adw_what htm 11 of 15 15 02 02 09 33 45 ADw what is ADHOCw for i 0 i lt Ix i itab i i tab i i writing the 2D data pixel for j 0 j lt ly j Iseek lu_int 2L Ix j SEEK SET write lu_int itab 2L Ix Iseek lu_float 4L Ix SEEK_ SET write lu_float tab 4L Ix closing files close lu_int close lu_ float delete itab delete tab Example of program in C for 3D cubes and integers 2 and floats 4 int Ix 50 ly 60 Iz 24 i j k float tab short int itab tab new float IZ itab new short int Iz opening output files lu_int sopen int idl O_BINARY O_RDONLY SH_DENYNONE lu_float sopen int float O_BINARY O_ RDONLY SH D
318. nserted after the page 1 of adwi_a htm adwi_f htm adwi_b htm adwi_c_htm adwi_d htm adwi_gen htm landscape printing inserted after the page 1 of adwi_d htm adwi_e htm file C ADHOCw HELP adw_man htm 3 of 4 15 02 02 09 35 07 ADHOCw Users manual gt page 10 of adhocman doc Table of contents coloured paper if possible gt pages 11 to 13 of adhocman doc detail of the table of contents Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_man htm Return to main ADHOCw menu file C ADHOCw HELP adw_man htm 4 of 4 15 02 02 09 35 07
319. nt Save file C ADHOCw HELP adwa2d_f htm 2 of 3 15 02 02 09 33 53 ADw2D image modifications Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_f htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_f htm 3 of 3 15 02 02 09 33 53 ADw2D 3D profiles ADw2D Return to main ADHOCw help Return to main ADw2D help Superposition modification of 3D profiles The Parameters folder gives the possibility in the 3D files section to define up to three 3D files for the superposition of the profiles on the 2D image The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page file C ADHOCw HELP adwa2d_e htm 1 of 8 15 02 02 09 33 54 ADw2D 3D profiles an ADC ranira 2 iva wesmex Wina Shan ADI IDC 21D display S Eiei LAr P Sexp eines M in Re ssxa cc 7 He af Wa th pear
320. nt of the channel are displayed You can change the cursor size default 1x1 pixel in this case the pixel content will be the mean value of all the pixels included in the enlarged cursor Profile area Moving the mouse in the 3D channel image area allows to obtain the local profile integrated in the square currently defined for the zoom If the square is 7x7 for instance the profile of 49 pixels will be added and displayed A tic small vertical mark in the upper part of the graph indicates the position of the channel where the mouse is located Actualize display useful function to get at any moment the image corresponding to the displayed parameters Load a new 3D file reloads a new 3D file only for AD3 DA3 mode Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite file C ADHOCw HELP adw3d_a htm 3 of 4 15 02 02 09 34 10 ADw3D main 3D display screen HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw3d_a htm Return to main ADHOCw menu Return to main ADw3D menu file C ADHOCw HELP adw3d_a htm 4 of 4 15 02 02 09 34 10 ADw3D interf full size Cube dim
321. ntinuum RV maps Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c3 htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_c3 htm 4 of 4 15 02 02 09 34 52 ADwT1 Finesse ADwT1 Return to main ADHOCw help Return to main ADwT1 help CO9 Calibration Finesse M ADw Finesse ADHOCW pesse ofthe calibration Input 30 file calibration Input 2D parabolic phase Choose file E ADHOCwS plus BLAISOUSPhas prh AD2 Zone of integration 1 192 1 192 to 2 30 Yalaz wa Execute 3 Help x Abort This function cannot z i be run m batch sate one te Ai Prini ine grapi file C ADHOCw HELP adwt1_c9 htm 1 of 5 15 02 02 09 34 52 ADwT1 Finesse Pantera pi Sarr grapi mO BMF DONS Tinton The user indicates the calibration cube and the phase The integration is within an area in which the bounds are computed If the phase value of a pixel is a null value the profile of the pixel is not taken in account in the computation The input file can be of
322. o X left and X right these parameters are important When the continuum spectrum is recognized in the F01 function its length could be smaller than the object spectra When computing wavelength for the object it is often necessary to extend the tabulated spectra geometry to the left and to the right without superposing spectra 1 Calibration parameters Input 2D calibration file in case of Pytheas this is the sum of all the continuum channels Threshold this threshold must be defined in order to separate TOTALLY the lines use ADw2D to find this value Height of measure for one spectrum pixels for calibration it is not necessary to integrate the full height of the spectra Smaller height avoid superposition between different spectra This value if the pixels to add upper and lower the central line of the spectrum 0 means 1 pixel in height only central 1 means 3 pixels in height central 1 2 means 5 pixels in height central 2 aso Sense of wavelength values increasing or decreasing from the left to the right Calibration wavelengths use function H10 to get exact wavelength values Polynomial degree is the degree of the dispersion curve file C ADHOCw HELP adwt1_f2 htm 3 of 8 15 02 02 09 34 33 ADwT1 TIGER 2 2 Elimination on calibration positions Sigma deviation the position of successive calibration lines is computed for every micro lens If the distance between two successive lines is ab
323. o draw crownsfr press Redraw graph Graph parameters 1 all 4 quadrants i POINTS real color lt l E crowns f4 Rmin 128 0 pix Vin 350 0 km s Aimax 128 0 pis Vmsx 2500 km s More zoom A Redraw graph Shift bald AV points When pressing the Minimize PA r Vs r and incli r button the following window will appear ap amp Dw2D minimizing parameters Pi joj x ADw2D optimizing crowns parameters for rotational velocities Symetrize radii Numer of crowns 10 Let vary Xe now fixed Xc Ye center of the curve Let vary Ye now fixed 1130 00 Let vary MA fr now fixed 155 00 MA position of the major axis in degrees direct sense 0 at top Let vary Vs r now fixed 1000 00 Vs systemic velocity in km s Let vary incli r now fixed 30 00 Incli inclination in degrees with respect to the sky plane Nb of iterations Aie 7a Results Crowns nb points bestxe bestVe bestmA bestVs bestinci sigma Vrot mean viot 4 file C ADHOCw HELP adw2d_k2 htm 8 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns Crowns nb points bestXc bese best MA sigma Vrot mean Vrot A E Save results into TXT file WARNING The computation time varies as the number of iterations The computation time can be huge if the number of iterations is important We recommend to the user to begin with a small number of iterations Note 1 Global optima
324. of the recorded photons Y addresses For DALSA AsGa it is usually the same value that CCD Y size there is no interest to decrease the size of the photon addresses witch can be binned later by software For Thomson this value is 256 Frames per second is used to compute the elementary exposure time and also the photon counting efficiency based on the frame count This value is 25 for Thomson 40 or 80 high rate for DALSA AsGa 512x512 and 20 or 40 high rate for DALSA AsGa 1024x1024 High rate DALSA AsGa is obtained via a switch on the DALSA camera itself ADw3D binning display allows to the display program ADw3D called by ADwIPCS to bin observations for quick look This function is interesting for 1024x1024 in order to get sufficient S N for the display If there is no binning put the value 1 DALSA high rate swap indicates to the program to correct the addresses with a X swapping in the right part of the image for DALSA AsGa camera This is due to the fact that the high rate frames per second doubled uses 2 output devices and that the second produces a X mirror effect For ADLSA AsGa high rate frames per second put 1 For all other cases put 0 Matrox driver for camera is a DCF file indicating the acquisition driver for the camera The following DCF files are normally present in the ADwIPCS EXE directory CCIR_N DCF 256x256 non interlaced Thomson camera CAD41K1T DCF DALSA CAD4 camera for AsGa Matrox
325. olating profiles 0 values gt mean A sigma 1 values lt mean A sigma 2 values gt mean A sigma and values lt mean A sigma evs osmiion nade 0 normal value channel p 1 mean of the 2 derivatives sigma A value iter nb of iterations oper type of selection operation Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0177 01 Lower 10 07 53 Operation Replace values gt meanta sigma 0177 01 Lower 10 07 53 with a 5 000000 and nb_iter 2 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1b12 htm file C ADHOCw HELP adwt1b12 htm 4 of 5 15 02 02 09 34 44 ADwT1 sorting eliminating interpolating profiles Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1b12 htm 5 of 5 15 02 02 09 34 44 ADwT1 continuum substraction ADwT1 Return to main ADHOCw help Return to main ADwT1 help B13 Suppression of continuum at pixel level This function s
326. ontains the sum of all the log books of the successive sessions For that press the Show logbook button above at any time file C ADHOCw HELP adwt1_c htm 1 of 3 15 02 02 09 34 51 ADwT1 menu CIGALE C01 Compute 2D phase map C02 Compute wavelength 3D maps C03 Compute monochromatic continuum radial velocities line widths 2D maps C04 Substract OH and or continuum from given areas C05 Get photometric parameters from OH lines case of CCD C06 Get seeing analysis channel channel case of CCD C07 Merging several ADS seeing parameters files C08 Photometric correction channel per channel from seeing ADS files C09 Compute the calibration Finesse C10 Build custom made lambda cubes C11 Get photometric parameters from rough analysis of non dephased channels C12 Continuum substraction from given area Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_c htm Return to main ADHOCw menu file C ADHOCw HELP adwt1_c htm 2 of 3 15 02 02 09 34 51 ADwT1 menu CIGALE Return to main ADWT1 menu
327. or SE file Choose file C cordnates of the array are included in the conection Correct columns Correct channels Ex Sto BOR overlapping 19 to 2 Use an execution mask Help X Abort E Store macro file C ADHOCw HELP adwt1b14 htm 1 of 4 15 02 02 09 34 45 ADwT1 correction of wrong lines columns channels The input and output files can be 2D or 3D The program recognizes automatically the type of the input file The user must notify the input file and the output corrected file The program can correct wrong lines or columns or channels If the user needs several types or correction the program must be run several times An array at the right of the dialog box allows to define at maximum 5 corrections lines columns or channels Bounds are included in the correction For channels note that if K2 lt k1 channels from k2 to k1 through 1 are selected 19 6 is the inverse of 7 18 The interpolation is linear The is no test on the null values The input file can be of new ADHOCw type AD2 or AD3 or old ADHOC type AD2 or DA3 The output file is created as new ADHOCw type AD2 or AD3 This function can use an execution mask When the execution mask doesn t allow the operation the extracting value is set to a null value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared between seve
328. or is jerry iss u net com You can also easily print your complete copy of the User s Manual Additional information structure of the ADHOCw files file C ADHOCw HELP adw_what htm 6 of 15 15 02 02 09 33 45 ADw what is ADHOCw This document describes the different formats which are managed by the program ADHOCw File Translator 1 New ADHOCw format 2 Old ADHOC Visu2 Visu3 format 3 Elc compressed format 4 IDL and binary formats In this section examples to read or write data are given for Fortran or C programmers 5 FITS format 1 New ADHOCw data format The new ADHOCw data format will be the default files format for the new ADHOCw software Windows95 WindowsNT The new ADHOCw structure has been defined in order to optimize the read write operations from to the hard disk a Principle the format is identical for 2 D and 3 D data data are stored as 4 bytes floating values 3 4E381 to 3 4E381 parameters and comment are stored at the end of the file default suffixes for the new ADHOC files are AD2 for 2 D and AD3 for 3 D b Differences with the old ADHOC VISU2 VISU3 format data dynamics is no more limited to 32767 32879 comments can now be 127 characters 78 previously separate parameter files are no more used size of the files is twice the previous c Compatibility the structure is simple in order to read easily ADHOCw files from user s programs written in Fort
329. ortant note 1 Only the visible points or crowns are used in the computation Nothing which does not appear on the graph is included in the computation excepted additional points see further Important note 2 If the individual pixels are drawn all the points have the same weight 1 If the crowns are drawn the weight of the crowns is the number of pixels integrated on the crown without_null values file C ADHOCw HELP adw2d_k1 htm 7 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph n this is the degree of the polynomial curve A degree 1 is an horizontal line constant A degree 2 is an oblique line A degree 3 is a parabola Curve type can be V r a0 at r a2 r 2 a3 r 3 V2 r a0 a1 r a2 r 2 a3 r 3 V r r a1 a2 r a3 r 2 a3 r 3 VA2 r r a a2 r a3 r 2 a3 r 3 Additional points to enforce zero or asymptotic values it is possible to add points with weight If this box is checked the define points are included in the computation If it is not checked only visible drawn points are used Define points by pressing this button the following window appears i ADw2D curve ICO x Additonal points for curve computation The user can add points in order to enforce the curve zero point asymptotic point These points are not drawn on the graph but are taker in account for the curve computation To suppress one point simply put the weight to 0
330. orting eliminating interpolating profiles ADHOCw Input 3B file Output 3B file Choose file Operation mode Value is the simple value of every channel Value is the mean of the 2 derivatives CCD cosmics Modify interpolate hi Value of A values gt mean A sigma Bo values lt mean A sigma Tales gt MEn Aaa A eean AED Nb of iterations 1 values gt mean A sigma and lt mean A sigma Ed l 2 For cosmic raps A 3 or 4 and Nbitet 2 is suggested Use an execution mask 4 Execute Help X Abort The input and output files are 3D The first operation mode simply takes the values for every channel The second one is better adapted to CCD cosmics the value which is checked is the mean of the 2 derivatives For instance if values for channels 10 11 and 12 are 1200 1500 and 1400 the value which is checked for channel 11 in the first mode is 1500 compared to all channel values but the value checked for channel 11 in the second mode is 200 1500 1200 1500 1400 2 200 The values are interpolated if they are strictly higher of lower than the value mean A sigma The interpolation is linear If several successive channels must be corrected they are computed independently from the 2 external channels which are inside the fork Store macro file C ADHOCw HELP adwt1b12 htm 2 of 5 15 02 02 09 34 44 ADwT1 sorting eliminating int
331. other basic photometrical or geometrical effects In this case a k 1 a k and B k b k a k These values are stored in the ADX output ASCII file which can be immediately used to do the correction file C ADHOCw HELP adwt1_c5 htm 2 of 11 15 02 02 09 34 46 ADwT1 photometry from OH The pixel beam is the size of the surrounding area where the profiles are added in order to increase the signal to noise ratio 3x3 or 5x5 are usually correct High values increase the computation time as the square of To determine this parameters it is recommended to visualize the input 3D profiles with ADw2D and to integrate several pixels with the ADw2D profile function The integrated profile must show if possible a pattern which is usually a night sky line The background noise cut allows to cut the lower values 0 15 means that the 15 lower values are not taken in account in the computation they appear as green points in the BMP graphics The high level cut allows to cut the upper values 0 90 means that the 90 upper values are not taken in account in the computation they appear as green points in the BMP graphics The micro phase correction is the possibility to correct the profiles from the variation of the phase inside the pixel beam Theoretically this correction must be done but the first data reductions show that better results are obtained when this checkbox is not checked One of the possible reasons is that the profiles are in
332. ouse inside the 2D image itself the replacement value will replace the original values nevertheless this will affect only the 2D image memory The modification of the display is immediate To modify later the 2D file itself the user must press the Save modified 2D file 1 button Replacement operation indicated the operation A old_value B that will replace the previous in the image If A 1 and B 0 the value remains unchanged Set value to NULL sets the replacement value to 3 1E38 null value Undo 2D successive modifications this is the way to undo previous modifications Up to 10000 modifications can be recorded and retrieved in case of error Left right top bottom extensions of the modification if one of these check boxes is on all the pixels which are located on the left right top bottom are changed This allows the user to clean very quickly an image which will be too long to clean only with the cursor size Save modified 2D file 1 saves the image memory into the 2D file 01 Other 2D files remain unchanged The pixels which are modified are all the pixels included inside the cursor box All these pixels will be put to a unique replacement value If the user forgets to save on disk the modifications which were done in memory when living the program the following window will appear 2h ADw2D Save2D EE The 2D image file 01 was modified but not saved onto disk Do you wish to save it before closing x Ho da
333. ove value of the lowest channel in case of emission or value of the brightest channel in case of absorption The continuum is computed separately Be careful the mode from intensity histogram can give high values if the line is not well defined the increasing slope will occur very near the maximum At the beginning use the default mode mean of the 3 lowest channels which gives every time a good result The radial velocities and line widths are both computed at the same time If the profile has several maxima or some other measurement problems occur the result value for the radial velocities and line width are set to a null value The monochromatic flux is computed from the threshold used for the profile analysis when computing the radial velocities When there is no velocity the monochromatic flux is set to Zero The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD2 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network file C ADHOCw HELP adwt1_c3 htm 2 of 4 15 02 02 09 34 52 ADwT1 monochromatic continuum RV maps Macro definition Example MONORV fin D ADHOCws_plus BLAISOUS call_p ad3 fmono D ADHOCws_plus BLAISOUS Mono_ORG AD2 fcont
334. owing beginning from the maximum of the line the program looks on both left and right channels until he finds nb of channels successive channels which inverse the sense of the profile Default value for the parameter is 2 1 is better for not noisy profiles 3 could be preferred for very noisy profiles if the number of channels is sufficient fixed levels the parameter Mono channels indicates a way to measure the base of the profile If this value is for instance 20 this means that this base is defined by the value of the channel for which 20 of the channels are more intense in the case of emission and 80 are less intense In this case the simple barycenter of the line is computed above this level Slope is the default method If the profile has several maxima or some other measurement problems occur the result value for the phase is set to a null value The input null values are not taken in account in this computation The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created file C ADHOCw HELP adwt1_c1 htm 3 of 6 15 02 02 09 34 17 ADwT1 phase computation as new ADHOCw type AD2 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition Example
335. p Inhib shutter inhib THT IPCS Confi aan DEF file o s Load DEF to current Help on DEF config files HELP for the acquisition parameters identification The number of the observation can range between 0 and 999 The prefix is a character from 4 to Z which will be used for the data and log file names with the observation number The comment is written in the observation logbook with the timing of the scans Type of acquisition 2D image allows to acquire and display a single 2D image In this case nevertheless the structureof the 3D files is maintained apparently channels are scanned in order to allow a similar display gt ADwIPCS configuration files ADwIPCS Return to main ADHOCw help Return to main ADWIPCS help DEF configuration files The configuration DEF files contain the information of the acquisition system to use There are some predefined DEF configuration files CHILE DEP for Thomson IPCS 256x256 at ESO GHASP DEF for Thomson IPCS 2560x256 at OHP ESO512 DEF for AsGa IPCS 512x512 40 frames s at ESO OHP512 DEF for AsGa IPCS 512x512 40 frames s at OHP OBC512 DEF for AsGa IPCS 512x512 40 frames s at Megantic ESO1024 DEF for AsGa IPCS 1024x1024 20 frames s at ESO OHP1024 DEF for AsGa IPCS 1024x1024 20 frames s at OHP QBC1024 DEF for AsGa IPCS 1024x1024 20 frames s at Megantic But the user can also write his own DEF file and load it A typical DEF file i
336. parameters L distance between lenses pixels E AAUt 20 000 D Y sampling floating pixels Alpha Tilt angle degrees MN automatic origin Ko 530 Yo 257 Starting wavelength ngstroems CAIN CCS 4 Reference zero wavelength Reference object line for kinematics STE Angstroems Ending wavelength Angstroems Wavelength step Angstroems 5 Result Output 30 wavelength file Choose file D Pytheas sh152_jlg tigre sh152_tigre ad3 Outut ADP parameter file defined with the output 3D file ADwT1 TIGER 2 UAPA ZEE YENNY SPECA TS Ines PUSHI Lnoose me D Pytheasish152_jlg TIGER_measured_calib AD2 Outut ADP parameter file defined with the output 3D file D Pytheas sh152 jig tigreish152 tigre adp 2 Elimination on calibration positions Output eventual PYTHEAS coefficients Choose file DAP theasish152_jlg PYTHEAS coefficients ADH Sigma deviation in the distance between two sucessives lines 7 gt Numero of the most intense line from left to right if 0 no test a Store macro Output verification calibration cube similar output wavelenath file D Pytheas sh152_jlg tigre verif_calib AD3 Input TXT spectra position file this contains the information which was transmitted from the F01 function to build cubes The file is TXT because is could be edited manually to suppress spectra for instance between the execution of the F01 and F02 functions Spectrum extension t
337. pdate the values in this program ADwT1 Thanks It is recommended to check these values before scanning Save pe pe pe po us fon one one rome Meme nr CFHT 2 M gantic 2 Ser San Pedro Ma tir 2 3 2 660 2 424 2 528 2 504 2 746 2 464 917 10 385 9 446 9 852 9 773 10 719 9 615 9210 10 429 9 501 9 908 9 842 10 794 9 683 9 120 10 327 9 396 9 798 9 720 10 660 9 563 2 327 2 635 2 394 2 497 2 480 2 720 2 440 file C ADHOCw HELP adwt1_h9 htm 2 of 3 15 02 02 09 35 03 ADWwT1 Perot Fabry talons Log book results None Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h9 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h9 htm 3 of 3 15 02 02 09 35 03 ADwT1 Common wavelengths ADwT1 Return to main ADHOCw help Return to main ADwT1 help H10 Common nebular and calibration wavelengths Am Es 7 Help XM Quit 60 H10 ADw common wavelengths ADHOCw Common wavelenhhs Nesular wavelenifis H alph
338. ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 sum_cal D ADHOCws_plus BLAISOUS Sum_cal AD2 cal_rv DADHOCws_plus BLAISOUS Cal_RV AD2 x11 6560 000000 xc 257 50 yc 262 50 ellipt 1 00 center 1 elliptCCD 0 p_pf 1162 Imbd_p 6562 780 Imbd_cal 6598 953 Imbd_scancal 6598 953 Imbd_obj 6562 780 Imbd_scanobj 6571 640 minangle 0 000 maxangle 360 000 minradius 0 000 maxradius 99999 000 Principle of the macro syntax A coded batch function has a function name Ex SMOOTHXY or PHASE and parameters with assigned values Parameters and values are separated by an equal sign All the function end with a space and a semi colon Maximum length of a macro is 4096 characters Maximum length for the macro function code is 16 characters Maximum length for a parameter is 275 characters 16 for the parameter name 1 for 256 for the parameter value 1 space and 1 for The parameter value can be a string a floating constant or an integer constant Strings are not encapsulated with inverted comas Blank lines are neutral Functions can be cut into different lines without additional code the ending semi colon separates the file C ADHOCw HELP adwt1_ba htm 4 of 6 15 02 02 09 34 07 ADwTI1 batchs functions But the cuts must be put where spaces exist between parameters for instance FUNCTION paraml 1 param2 toto can be edited as FUNCTION paraml 1 param2 toto Comment lines Comment lines can be inserted in the text by the user The ar
339. pixel level for a 3D file B14 Correction of wrong lines columns channels of a 2D or 3D file B15 Photometric correction channel per channel from ADX file B16 2D image enhancement correction of non gaussian defects B17 2D or 3D mosaic B18 Spectral deconvolution 3D file B19 Spatial deconvolution 2D or 3D file Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1_b htm 2 of 3 15 02 02 09 34 36 ADwT1 menu OPERATIONS 2D 3D Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b htm 3 of 3 15 02 02 09 34 36 ADwT 1 sum of the channels ADwT1 Return to main ADHOCw help Return to main ADwT1 help B01 Sum of all the channels ADw sum of all channels Iofs ADHOCw an of aff de chansers af a cuv e Input 30 file cube Choose file Output 20 file zum Choose file Fi Execute Help EX Store macro The user must only give the name of the 3D input file and the 2D output file which will contain the sum of all the channe
340. prb AD2 out D ADHOCws_plus BLAISOUS cal1_p ad3 gt Computation of wavelength maps lt ADHOCw Command 0249 Task 02 gt 3D input data file 70249 02 Lower 20 32 38 Starting function D ADHOCws_plus BLAISOUS Cal1 da3 acro LAMBDA fin D ADHOCws_plus BLAISOUS Cal1 da3 gt 2D input phase file ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 D ADHOCwS_plus BLAISOUS Phas_prb AD2 out D ADHOCws_plus BLAISOUS cal1_p ad3 gt 3D output data file 0249 02 Lower 20 34 05 Correct end D ADHOCws_plus BLAISOUS cal1_p ad3 70249 02 Lower 20 34 05 Ending function Suspend task Abort task EB Save results Print results The macro box indicated the executed macro The Execution parameters is in fact a more comprehensive explanation of the macro the macro is here decoded The Results is the logbook limited to this macro by comparison to the global logbook in the function windows of ADHOCw You can save this information on an ASCII file by clicking on the Save results button or print it by clicking on the Print results button It is necessary to close this window to access to information of another task The current global history ASCII file name ADL type is indicated in the bottom of the window Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly a
341. priorities photons s 842 total nb photons 000000600000 High frames s 25 written on disk 0000000 0 Mb Critic count efficiency100 total counting efficiency 0 F4 automatic from photon rate chs ie OOOO Iv this window always in front rene window See permet BB allow modification Discri Ro Black lul Fr i ers of the TV parameters def 20 def 51 Write on logbk The user must first start the acquisition by pressing onto the Start button the acquisition starts when the channel exposure counter counts seconds Current values appear in inversed maroon while acquisition parameters appear in inversed blue The left upper part displays the number of the observation the photon counting status and the possible directives to stop the acquisition Instantaneous photons s counted photons per second frames s frames detected per second counting efficiency must be as near 100 as possible High fluxes decrease the efficiency Cycles and channels channel exposure in seconds is incremented at every successive scan current channel indicated the current exposed channel A sign gt gt gt gt gt or lt lt lt lt lt indicates the sense of channel numbering see saw current cycle scanning wavelength from acquisition parameters Queensgate constant from acquisition parameters Cumulated gives the statistics System priorities allows to control the Window NT system ADw syste
342. pted the text of the macro and the ending execution message the following information is recorded 0176 01 Lower 09 36 13 Files are F1l amp F2 input F3 output 0176 0Ol Lower 09 36 13 Operation F3 Fl F2 A B 0176 0Ol Lower 09 36 13 with a 1 000000 b 0 000000 file C ADHOCw HELP adwt1_B7 htm 3 of 4 15 02 02 09 34 40 ADwT1 mixed arithmetic operations and c 0 000000 Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b7 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_B7 htm 4 of 4 15 02 02 09 34 40 ADwT1 spectral smoothing ADwT1 Return to main ADHOCw help Return to main ADwT1 help B08 3D spectral smoothing The original figure of the menu being large it has been reduced to fit in a printable page and in classical screens Click here to visualize the figure with full resolution for help manual on paper see next page p AN w amend alaf aa IE T1 ADHO Cw AT So ee Fika apit Uk Choose file Jup SO lie
343. put control TXT file Choose file Jbx_portable D ADHOCWS plus BLAISOUS OH TXT Use a reference photometric 2D file i OH profile Nb of pass E Substraction factors tat 1 M Continuum suppression no suppression C total suppression at last pass C partial suppression at last pass Build and correct interactively graphically the OH profile C Use the rough OH profile computed in the zones without nteraction WJbx_portable D ADHOCWs_plus BLAISOUS PROFILOH AD1 Pa Execute Help X Abort EX store macro Output AD1 profile file Choose file Use an execution mask file C ADHOCw HELP adwt1_c4 htm 1 of 6 15 02 02 09 34 15 ADwT1 OH and or continuum substraction The user must notify the input 3D the output 3D file and the ADZ zones file The input data file can be of new ADHOCw type AD2 or old ADHOC type DA2 The output data file is created as new ADHOCw type AD2 The ADZ zone file is issued from the ADw3D zone function and is an ASCII file containing the x1 y1 x2 y2 coordinates of the area to take in account At the end the coordinates are rearranged in order to have x2 gt x1 and y2 gt y1 but the original file is not changed The ADZ zones file is compatible with the old ADHOC DOS area files functions 13 and 48 The only change is that the coordinates can be now float and not limited to integers O or 999 values are not taken in account as well that comm
344. put file name with whole path chnl number of the channel to extract numbered from 1 Log book results Excepted the text of the macro and the ending execution message no information is recorded Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1_b2 htm 2 of 3 15 02 02 09 34 37 AdwT1 extraction of a channel Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b2 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b2 htm 3 of 3 15 02 02 09 34 37 ADwT 1 insertion of a channel Return to main ADHOCw help Return to main ADwT1 help B03 Insertion of a channel into a cube ADw insert channel Iofs ADHOC w sert amp channel info G cube Input 2D file channel image Inputoutput SD file cube modify Choose file Channel number to extract fi Use an execution mask Execute 7 Help x Abort amp Store maero The user must only notify the input 2D file which contains the image of the channel the output cube which will be modified and the channel number number
345. r 21 6581 00 900 4800 630 280 1000 167 400 562 2 verifier y 436300 800 4000 940 000 2300 4 00 400 500 2 verifier 23 y 4865 72 1080 5600 820 0 00 26 00 1 67 400 5 62 2 verifier F uai 1 Ot mme ame me anm mme dnm ame mme ni te The user can select a list of filters from an ASCII file previous list stored at every execution of the program ADHOC generic filter list ASCII file adw_lIfi txt external user filter list file C ADHOCw HELP adwt1_h8 htm 2 of 6 15 02 02 09 35 02 ADwT 1 Interference filters The user can set active or not active each one of the filters by clicking with the left mouse button on the active box relative to one of the filters This function is toggle Then to see the curves press Execute a ADw filter curve DIX ADHOCw Afer curves tzid emcees DiameterM1 DiameterM2 Focallength cm from telescope identification 3m60 ESO Cass F 8 La Silla gt 356 60 120 00 2865 00 F8 C from aperture ratio C from mean inclination angle Mean inclination degrees 2 642 Object parameters Temperature Drawing scales Compute wavelength from Lambda 0 6562 780 Angst Name radial velacit 20 0 6560 0 TOTO Seale a Racal vel 1261 000 km s is M Filters 6610 0 Wavelength Anastroems observed Mano 2 redshift 0 000 L e Lambda max SE on en Selected lambda 5610 000 Angst al fiters Ztrensm mas 20 0 X Quit Help IF TOTO lambda 6590
346. r the page 1 of adw3d_a htm adwtl htm adwtl_ge htm adwtl_gf htm adwtl_ad htm adwtl_fc htm adwtl_ta htm adwti_di htm adwtl_ma htm adwtl_ba htm adwtloth htm adw_supp htm adwtl_a htm adwtl_al htm adwtl_a2 htm adwT1_a3 htm adwt1_b htm adwt1i_bl htm adwt1_b2 htm adwt1_b3 htm adwt1_b4 htm file C ADHOCw HELP adw_man htm 2 of 4 15 02 02 09 35 07 ADHOCw Users manual adwt1_b5 htm adwt1_b6 htm adwt1_b7 htm adwt1_b8 htm adwt1l_b8t htm landscape printing inserted after the page 1 of adw3d b8 htm adwt1_b9 htm adwt1_b9t htm landscape printing inserted after the page 1 of adw3d b9 htm adwt1b10 htm adwt1b11 htm adwt1b12 htm adwt1b14 htm adwt1b15 htm adwt1b16 htm adwt1b17 htm adwtl_c htm adwt1i_cl htm adwtlcit htm landscape printing inserted after the page 1 of adw3d_cl htm adwt1i_c2 htm adwt1i_c3 htm adwt1i_c4 htm adwt1i_c5 htm adwt1i_c6 htm adwtl_c7 htm adwtl_c8 htm adwt1i_c9 htm adwt1c10 htm adwt1c11 htm adwt1i_d htm adwtl_e htm adwtl_el htm adwt1i_f htm adwt1_f1 htm adwt1_f2 htm adwt1_g htm adwt1l_gl htm adwt1i_h htm adwt1_h1 htm adwt1_h2 htm adwt1_h3 htm adwt1_h4 htm adwt1_h5 htm adwt1_h6 htm adwt1_h7 htm adwt1i_h8 htm adwt1i_h9 htm adwt1h10 htm gt page 9 of adhocman doc 7 Program ADwIPCS coloured paper if possible adw_ipcs htm adwi_a htm adwi_it htm landscape printing i
347. ral process or users and can be located on other computers accessible on the network Macro definition Example Macro CORRECT fin E ADHOCws_plus BLAISOUS bidon ad3 fout E ADHOCws_plus BLAISOUS bidon2 ad3 oper 0 froml 5 tol 9 from2 35 to2 35 from3 40 to3 50 keyword content options CORRECT i file C ADHOCw HELP adwt1b14 htm 2 of 4 15 02 02 09 34 45 ADwT1 correction of wrong lines columns channels fin 2D or 3D input file name with whole path fout 2D or 3D output file name with whole path oper type of operation 0 correct lines 1 correct columns 2 correct channels Note that from or to not used values are not needed in the macro Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0178 01 Lower 10 41 58 Files are 3D 0178 O01 Lower 10 41 58 Operation Correction of wrong lines 0178 01 Lower 10 41 58 zone 1 from 5 to 9 0178 01 Lower 10 41 58 zone 2 from 35 to 35 0178 0Ol Lower 10 41 58 zone 3 from 40 to 50 Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adwt1b14 htm 3 of 4 15 02 02 09 34 45 ADwTI1 correction of wrong lines columns channels Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly
348. ran or Basic without parameters amp comments the structure is IDL compatible without parameters amp comments d C library a C object oriented C library is available for users binary and C code e Structure data Ix ly lz 4 bytes Ix ly and Iz are the dimension of the cube lz 0 for 2 D parameters 128 bytes comment 128 bytes gt So the total length of the file is Ix ly 1z 4 256 bytes f Coding as coding is different from PC and UNIX machines the 4 first bytes of the parameters which contain an integer value representing the number of dimensions of the data will be used as test g Parameters all values are 4 bytes integers floats or character blocks all integers are long integers 4 bytes 10 first values are common for 2 D and 3 D files other values are specific to these different files values are compatible with old ADHOC files DA2 and DA3 For all files 2D and 3D file C ADHOCw HELP adw_what htm 7 of 15 15 02 02 09 33 45 ADw what is ADHOCw ocation bytes type mnemo description default 0 3 integer nbdim nb of dimensions 3 4 7 character lid1 identification 1 2 P 7 11 character id2 identification 2 2 P 2 15 integer Ix dimensioninX 256 16 19 integer lly dimensioniny 256 20 28 integer z dimensioninZ 24 24 27 float scale arcsec pixel 1 8 31 integer jixO lop leftcomer lo 32 35 integer iyo lbottom rightcomerO 86 39
349. ration F2 8 F1 B F2 alogi0 F1 A B F2 InfF1 A B F2 10 F1 A B F2 exp F1 4 6 F2 4 F2 sort F1 4 6 F2 FA 2 B 4 Execute P Help The program accepts 2D or 3D files it recognizes automatically the type of the input file The user has the following possibilities in which F1 and F2 represent two 2D or 3D files F1 is the input file and F2 is the output file F2 A Fl B file C ADHOCw HELP adwt1_b5 htm 1 of 4 15 02 02 09 34 39 ADwT1 arithmetic operations F2 alog10 F1 A B F2 ln F1 A B F2 10 F1 A B F2 exp F1 A B F2 A F2 sqrt F1 A B F2 F1 A 2 B The user must provide the names of the input and output files and the values of the floating variables A and B It is possible to set A or B to a null value 3 1E 38 by pressing the corresponding button If the result is less than 3 1E 38 the value is set to 31E 38 null value If the result is more than 3 1E 38 the value is set to 3 1E 38 The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output file is created as new ADHOCw type AD2 DA3 This function can use an execution mask When the execution mask doesn t allow the operation the cube value F2 will be set with the F1 value This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween sever
350. re niring gi ee o measa e l Bes a Aa r stesqere xi 1512 gt Lin oA We ans in NA wan 1 vs cod ey 2 LECLE EN Shanti A da con Hi ss LA te pein ve lasi ot mnt amp vw file C ADHOCw HELP adw3d_b htm 1 of 3 15 02 02 09 34 12 ADw3D main 2D display screen Page folders You can access to two pages folders Interferograms 3D display and Sum this 2D display ZOOM The image area can be easily zoomed The simplest way is to click on the right button on the mouse it will be a zoom x 2 centered at the mouse location Similarly you can unzoom of a factor 2 by clicking on the right button of the mouse but pressing at the same time the shift key Another way is to change the Image area box which gives the size of the displayed image Graph area change this to display all the channels at the same time Field You can move the field by changing the X0 and YO values Palette You can change the color palette different rainbows black and white color inversions Step threshold and scale overlap The correspondence between the values of the image and the colors is obtained from 3 parameters the threshold lowest displayed value the step space between colors and the possible overlap If there is no scale overlap all the values larger than the last step are displayed like the last step If the scale overlap checkbox is checked there is a modulo to compute
351. re pes oo a oo ges Hes eps este pr rdedevepers xi SIS 42332170 442201 SEV SER LP NA iron ede Aol ioni alan Shanti A TE LETT thew i LA te pein vo ce Ste HE hedwht 10 at oe muy vuaj Dee 11 vra rewia E He ar Sener hh Jadtraiett 1e ECS TE C n RUNAIR It is possible to save the zone coordinates into a ADZ file which can be read by the ADwT1 program To display the profiles the user can define the spectral domain by indicating the starting and ending channels to display the option to show or not the continuum the possibility to normalize profiles all over the 11 zones or only per zone When the user puts the mouse on a profile a vertical cursor appears in all the existing zones and the number of the channel is displayed in the upper right part of the image area The profiles can be stored as ASCII file in the AD1 format The values are in intensity per pixel Here is an example of the AD1 format 000000 Zone 500726 Zone 516999 Zone 506340 Zone 494154 Zon 480061 Zone 470169 Zone Jo U amp amp ND H PRPPRPRPRP PR PPP PRP RPP file C ADHOCw HELP adw3d_c htm 2 of 3 15 02 02 09 33 57 ADw3D 11 zones 8 1 464281 Zone 1 9 1 457071 Zone 1 10 11 12 13 14 15 16 17 18 19 20 Al 22 23 24 25 26 27 NPRPRPPRPRPRPRPRPENNFPRPRE EB 458226 Zone 1 478108 Zone 1 528030 Zone 1
352. reference file if mode_ref 1 fomp output BMP control file file C ADHOCW HELP adwt1c11 htm 4 of 8 15 02 02 09 34 53 ADwT1 rough photometry bkgd background to substract from individual channel profiles Log book results Excepted the text of the macro and the ending execution message the following information is recorded ADHOCw Command 0173 Task 01 0173 O01 Lower 17 58 13 Starting function Macro ROUGH PHOTOM fin D Data IKI neb2_cos ad3 fzones D Data IKI zones2 adz mode_ref 0 fphotom D Data IKI truc adx fbmp D Data IKI truc bmp bkgd 0 0173 01 Lower 17 58 13 Zone l x1 49 000000 y1 119 000000 x2 158 000000 y2 183 000000 0173 01 Lower 17 58 13 Zone 4 x1 31 000000 y1l 248 000000 x2 90 000000 y2 338 000000 0173 01 Lower 17 58 13 Zone 8 x1 395 000000 y1 296 000000 x2 463 000000 y2 381 000000 0173 01 Lower 17 58 13 Zone 11 x1 352 000000 y1 131 000000 x2 463 000000 y2 202 000000 0173 01 Lower 17 58 18 nb pix in the 4 zones 26608 26608 0173 01 Lower 17 58 19 k tabz ref 0 912 281189 0173 01 Lower 17 58 19 k tabz_ref 1 912 271973 0173 01 Lower 17 58 19 k tabz_ref 2 912 317261 0173 01 Lower 17 58 19 k tabz _ref 3 912 366943 0173 01 Lower 17 58 19 k
353. remanence You can also have a quick view of the ADA integration from the ADw3D program from CFHT CCD The format is FITS You must use the 2D slices gt 3D translation in the ADWFT program Note the possibility to assign directly the channels numbers with the Automatic CFHT ordering checkbox in the 3D slices translation window from Byurakan CCD The format is FITS You must use the 2D slices gt 3D translation in the ADwFT program Note that you will be able in further versions to compensate the seeing and transparency variation all along the exposure by using the guiding CCD log file For the moment use the old DOS procedure for that file C ADHOCw HELP adwft_a3 htm 1 of 2 15 02 02 09 34 05 file C ADHOCw HELP adwft_a3 htm from SAO photon counting The format is TRIM 512x512 which is similar to ADA 2 x 2 bytes You can directly integrate the data from the ADw3D program Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft_a3 htm Return to main ADHOCw menu Return to main ADWFT menu file C ADHOCw HE
354. rification file zero wavelength calibration interference order D Pytheas sHi1 5A pytheas PYTHEAS zero wl AD2 Execute Help x Abort Store macro 1 Spectra position parameters Input PYTHEAS coefficients this is a binary file is transmitted by the F02 function and contains all the information on the spectra position dispersion 2 Calibration parameters Input 3D calibration file 3 Object parameters Approximated interference order at a given wavelength this is only an approximated value because the program will compute the exact value around the given value 5 Don t compute exact interference order as the etalon could be badly tuned interference order could vary in the field In this case the computation of the exact interference order could be wrong In this special case the user can fix the value The approximate value given above will be used instead of the computed one Scanning wavelength for object and calibration in fact this parameter is not used during file C ADHOCw HELP adwtt_g1 htm 3 of 14 15 02 02 09 34 35 ADwT1 PYTHEAS 1 data reduction but value must be theoretically larger than the ending sampling wavelength to complete totally the spectral information 4 Sampling parameters Starting wavelength ending wavelength and step define the wavelength sampling Integrate pupil spot along the spectrum if it is checked the program takes in account that
355. ry of the macro command file if running macros If no default directory is mentioned and no macro is running the full path must be given in the fin and fout parameters of the FILTRANS commands FILTRANS transtype tin inputtype tout outputtype fin filenamein fout filenameout Ix dimx ly dimy nc nbchan first chan1 cfht valcfht a facta b factb FILTRANS is the identification of the command transtype string ex 3D3D 2D2D 3Ds or s3D 3D3D 3D gt 3D 2D2D 2D gt 2D 3Ds 8D gt 2D slices s3D 2D slices gt 3D inputtype format of the input file integer outputtype format of the output file integer file C ADHOCw HELP adwft_d htm 2 of 6 15 02 02 09 34 09 ADwET Macros and batch filenamein name of the input file filenameout name of the output file eventual parameters are Ix and ly dimensions X and Y integers in the case of binary IDL inputs and slices inputs nc number of channels integer in the case of 3D binary IDL inputs and slices inputs first number of first identification channel integer default 1 in the case of input 2D slices valcfht 1 if CURCHAN ordering requested integer 0 default if not in the case of input 2D FITS slices a normalization factor float b normalization factor float inputtype for 3D files 0 ADHOCw default AD3 PC or Unix float32 spectra 1 ADHOC old VISU3 DA3 int16 spectra 2 EIC compr
356. s 32 Binary or IDL Unix integers Binary or IDL Unix floats 32 FITS 3D FIT FITS 3D FIT FITS 3D FIT integers FITS 3D FIT integers FITS 3D FIT integers FITS 3D FIT integers FITS 3D FIT integers FITS 3D FIT integers ADHOCw Unix AD3 floats 32 ADHOCw Unix AD3 floats 32 8 ordered by spectra 8 ordered by channels 16 ordered by spectra 16 ordered by channels 32 ordered by spectra 32 ordered by channels swapped and by spectra swapped and by channels 2D input and output accepted formats file C ADHOCw HELP adwft_a1 htm 1 of 2 15 02 02 09 34 08 ADwET 2D and 3D translations Al DHOCw Al F Binary or Binary or Binary or Binary or F F F F A DHOC old ITS 2 D PC AD2 Floats 32 DA2 Integers 16 ak T FITS Floats 32 IDL PC Integers16 IDL PC Floats 32 IDL Unix Integers 16 IDL Unix Floats 32 T FITS Floats 64 ITS Integers 8 F T FITS Integers 16 FITS Integers 32 ITS 2D F TIS 2D PRIT ITS 2D F TS 2D FIT DHOCw Unix AD2 Floats 32 swapped Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended op
357. s Choose file Coordinates of the star in the first channel 108 T E Size of the analysis bow Bow size Store macra This function is supposed to compute automatically the seeing corrections X Y displacement and seeing value for CCD observations This function is only doing the analysis of the correction generating an ADS output ASCII file not the correction itself file C ADHOCw HELP adwt1_c6 htm 1 of 7 15 02 02 09 34 48 ADwT1 seeing analysis which must be done later The computation is done channel per channel So the 3D input file must be not dephased as original or corrected from flat field and or cosmic rays Coordinates of the star are numbered from 1 The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DAS The output ADS seeing parameter file is ASCII and has a special ADS format This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared between several process or users and can be located on other computers accessible on the network Macro definition Example SEEING fin E ADHOCws_plus BLAISOUS oba2 ad3 fseeing E ADHOCws_plus BLAISOUS bidon ads flbmp E ADHOCws_plus BLATISOUS bidon bmp xc 217 yc 200 box 21 Keyword content options SEENG XC X center coordinate of the star to analyze counted from 1 yc M center coordinate of the s
358. s SH152 sum_P040 ad2 fverif D Pytheas SH152 TIGER_extracted AD2 fpos D Pytheas SH152 TIGER_pos TXT fverif2 D Pytheas SH152 TIGER_selected AD2 felimin D Pytheas SH152 TIGER_eliminated AD2 threshold 3410 length 80 width 7 lmini 30 wmini 1 yc 0 000 xc 0 000 dxh 0 000 dyh 0 000 dxv 0 000 dyv 0 000 mode 0 geo 0 keyword content options TIGER POS fcont continuum 2D input file name with whole path PO fverif verification 2D output file name with whole path fpos output TXT position file name with whole path 0 fverif2 verification 2D output file name with whole path Pp 0 file C ADHOCw HELP adwt1_f1 htm 6 of 8 15 02 02 09 34 34 ADwT1 TIGER 1 felimin elimination 2D output file name with whole path threshold continuum threshold length maximum length i width maximum width Imini minimum length o wmini minimum width yc Y central position of the reference lens XC X central position of the reference lens dxh lhorizontal delta X dyh horizontal delta Y dxv vertical delta X dyv vertical delta Y mode lens array type 0 hexagonal lens array geo geometrical correction lo no Log book results H geometrical correction Excepted the text of the macro and the ending execution message the following information is recorded 0009 09 Lower 16 50 39 F01 TIGER_POS Info 0009
359. s a very simple browser file C ADHOCw HELP adwt1_h2 htm 2 of 3 15 02 02 09 34 18 ADWT1 translation of the phase to old ADHOC format incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h2 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h2 htm 3 of 3 15 02 02 09 34 18 ADwT1 menu GENERAL ADwT1 Return to main ADHOCw help Return to main ADwT1 help General functions A 2 ADw ADwT1 Pile x Bring task manager to front ADHOCw ADwT1 Version 994 ji a ete IJ FA 20 ppi 401 General parameters of the cubes 802 Tabulate wavelength and velocity values per channel 403 Heliocentric RY and precession computations gt Edit a batch file lt 3 Exec a batch file Display control Quit the program 7 Help Session log book see the ADL log file for the full history of all the sessions Suspend log book update for manual scrolling This log book is presently empty because you just begin this session You can also display the ADL ascii log file which contains the sum of all the log books of the successive sessions A01 function General parameters of the cubes file C ADHOCw HELP adwt1_a htm 1 of 2
360. s also ADw3D Eji i The indication below the executable file names represents the optimal screen size and colors X Abort New All programs are file sharing and network compatible You can run a program by double clicking on its name or by selecting it one clock only and then clicking on the Execute button The Help button gives you access to the global ADHOCw HTML help Note that the indication below the executable file names represents the optimal screen size and colors If your system doesn t offer such a screen or is the resolution is not 96 pixels per inch a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode file C ADHOCw HELP adw_what htm 3 of 15 15 02 02 09 33 45 ADw what is ADHOCw Note that several ADHOCw ADw2D ADw3D ADwT1 or ADWFT programs can run at the same time on the same directory same data or on different directories different simultaneous treatments Shared files and network access The ADHOC software manages completely the Windows networks you can access and write if permitted by the manager to any data file located on another computer All the files are completely shared in reading but locked only to one writing user at the same time A good example of the macro syntax for network input and output files can be seen in the ADwT1 function C04 Batches Data reduction program ADwT1 and File translation program A
361. s as following 6000 THT low level 9400 THT medium level 10800 THT maximum 20 Discri 50 TV black level 255 TV white level 0 CS100 interface 0 n COMn 0 shutter system O THT system 0 no control 99999v 512 CCD X size 512 CCD Y size 512 stored image X size 512 stored image Y size file C ADHOCw HELP adwi_f htm 1 of 5 15 02 02 09 34 01 ADwIPCS configuration files 40 frames per second al ADw3D binning display 0 DALSA high rate swap 1 yes Cele nace Matrox driver for camera vmi03_60 vcf Matrox driver for control display END THT low level is the THT voltage which is automatically reached as first step when tuning the very high voltage Usually there is no risk for the tube at this voltage even in case of bright illumination Photons usually don t appear THT medium level is the THT voltage which is automatically reached as second step when tuning the very high voltage Usually there is a risk for the tube at this voltage for bright illumination but not for common observations Photons begin to be visible THT maximum is the physical maximum THT voltage The user must control the flux on the TV control display and adjust the THT value with the observation brightness The risk is maximum Discri is the binarization level for the Matrox board This value must be tuned and set with the Test Matrox function TV black level is needed
362. s in order to get the expected information 14 smooth spectrally and or spatially the dephased files like LMBD AD3 If necessary use the execution masks 15 compute again monochromatic continuum radial velocities maps like explained above change only _ORG to another suffix 16 extract if needed with function B10 one local reduced area in order to minimize the computing time specially for smoothings and the file sizes file C ADHOCw HELP adw_proc htm 4 of 5 15 02 02 09 34 47 ADHOCw Typical reduction procedure Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw_proc htm Return to main ADHOCw menu file C ADHOCw HELP adw_proc htm 5 of 5 15 02 02 09 34 47 ADwT1 seeing analysis ADwT1 Return to main ADHOCw help Return to main ADwT1 help C06 Seeing analysis channel per channel CCD M ADw seeing analysis ADHOCw Seeng Onasis Channe channel CC Input original not dephased 3D file Choose file Output ADS ASCI seeing parameters tile Choose file Output control BMP tile name
363. s second display are marked with an asterisc but are not scratch because the possible absence of the second display This optional second screen display must manage A024R7 6S pixels minimum Simple message on screen Continous TY acquisition Grab a single 768x576 image in 402 format Grab a single 512x512 image in AD2 rat g mti ns lt allowsto TUHE TY 2 Move and test the PF interferometer Tune THT x Returnto program Shop Tunctiion Choose a function and execute file C ADHOCw HELP adwi_e htm 1 of 4 15 02 02 09 34 04 ADwIPCS tuning We suggest the following tests before acquisition These tests are accessible by pressing the Test Matrox and IPCS button on the parameters window 1 check that the MATROX board is working Run the Simple message on screen test If a message is displayed on the second VGA screen it is OK If the program answers that it cannot find the Matrox board you have an hardware problem 2 check the TV acquisition Run the Continuous TV acquisition test If the VGA screen displays the TV it is OK If nothing appends the most probable is that there is no TV synchronization Do you see any feature on the classical control TV screen Is the IPCS TV on not the intensification only the TV Is the coaxial cable connected to the Matrox board You can also look to the TV signal on an oscilloscope 3 check the interferometer Put THT on the int
364. s sections a Integration of profile val AL h P Flip vertivally PF Flip horizontally Image modification TEn overnay Rainbow C Kinematics of galavies E sh Histograms Image area Sess 160 a T 32x32 v Sem yg 50 Mini 0 000000 Maxi 4109 605957 x0 Yo 0 m Integrated profile ia 228 276 Sy Nb cells 5 a A NE pixels 45 Pafi w Clear selection AJAN pE n E Fejl Visualization mode 4 LA Square pixels Iu i i ES Al an Barycenter ta Current RY Chopped RY gt Copy to 2D image j H PR ne 0 Undo 2D successive modifications Modify replace and store profile IL Cni1 6560 00 J Actualize full display Db a ae 78A ju con He i 2 JAA om 0 00 km s Po NI Ln J H 4 Bi Lo ale j F Draw R tics on profile file C ADHOCw HELP adwadi4t htm 15 02 02 09 33 56 ADw2D zoom on profiles ADw2D Return to main ADHOCw help Return to main ADw2D help Zoom on profiles This function allows accurate measurements and zooms on details ADw2D integrated profile No smoothing zj Eull spectrum from 6520 000 to 6610 000 BaCENE Be chnl I jl E Lmbd TE Y from 400 6505 to 8208841 o i valchi RIES AV E he left mouse button 880 8841 file CI ADHOCW HELP adw2d_zp htm 1 of 7 15 02 02 09 33 56 ADw2D zoom on profiles 400 6505 La AN ANA AA 6520 000 6610 000 The Y value at cursor position the channel number the value
365. s tasks on other programs and modules So only one program gives the access to all functions its name is ADHOCW EXE The best is to run it from the shortcuts created during installation ADHOC software Version 2001E 10 apr 2001 FA ol x ADHOCw data processing software me Execution 418 ratte Observatoire de Marseille J Boulesteix http www obs_cnrs mrs ft ADHOC J Double click suggested How to update software ETAT eae New users click here ADw2D exe 2D display program TOME Da displays up to sh 2D files ADHOC or FITS farmal in supermposed or blink mode Up to three 3D files can also be ADw3D exe C 3D display program 1200510244256 ADw3D displays cube mosaics ADHOC or FITS format and profiles Ny manipulations It builds also 3D cubes from individual 2D files E ADHOCw ADwTlexe f Data reduction program Analyse et 800 600 16 a D pouillement ADwT1 is the 2D and 3D data reduction module multi tasking file sharing Homog ne des and network compatible Observations Cigale ADwFT exe File transfer program windows 32bits SEI IUNTS ADwFT allows numerous 2D and 3D file conversions ADHOC FITS binary including 2D 3D slices conversions Dumps header displays and Author Worldwide data modifications are also possible 7 ADHOC files suffi xes ADwIPCS exe C i isiti ie Photon counting acquisition program Help L ADwIPCS is a real time photon counting acquisition program which load
366. scape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_a htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adwa2d_a htm 2 of 2 15 02 02 09 33 48 ADw2D general functions ADw2D Return to main ADHOCw help Return to main ADw2D help General functions These functions appear on the upper part of the window and are available for any folder ER Export display to BMP E Setup printer Print Fe Save ADC conten 7 Hei X Quit the pragrarn Setup printer choose printer and orientation Print print the window on the current Window printer Save ADC context saves the current display parameters to a ADC context file Help get ADw2D help Export display to BMP save the current displayed image to a BMP image file In addition the user may also save the scale as BMP image file Quit the program quit ADw2D Comment or information boulesteix observatoire cnrs mrs fr file C ADHOCw HELP adw2d_y htm 1 of 2 15 02 02 09 33 48 ADw2D general functions Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special
367. se file Use an input 20 reference photometric file FT Create BMP graphic control output files eae ele sde nan ee eee eee gee eee epee eee peer dus Nunnan een en ent nana nn sense memes tn ne een nes Note Graphic control increases sional the execution time cf the program Background noise cut High level cut Pitel bearta increase SN ois pa 545 pixels ha LE A T Aaf Ee srs Wee 4 A irs file C ADHOCw HELP adwt1_c5 htm 1 of 11 15 02 02 09 34 46 ADwT1 photometry from OH F we 1 DoR GAA A A lal HAE E E LAA Piel bear to increase SAN GEEN i or i E5 pires _ px me jo 5 0 90 0 15 recommended 0 90 recommended D Corect micro phase not recommended for beams lt 545 i Help x Abort Store macro This function is supposed to compute automatically the photometric corrections sky transparency and sky night background for CCD observations This function is only doing the analysis of the correction generating an ADX output ASCII file not the correction itself which must be done later function B15 Important note if this method fails use the C11 rough method This method could fail if there is absolutely no significant OH pattern and or the variations of the background and transparency are too large compared to the recognizable pattern The principle is the following The computation is done only in special areas which are supposed to be pure background areas The best is
368. set to 3 1E 38 null value If the result is more than 3 1E 38 the value is set to 3 1E 38 The input files can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output file is created as new ADHOCw type DAS This function can use an execution mask When the execution mask doesn t allow the operation the cube value F3 is set to value of F1 This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network Macro definition file C ADHOCw HELP adwt1_B7 htm 2 of 4 15 02 02 09 34 40 ADwT1 mixed arithmetic operations Example ARITHM3 finl E ADHOCws_plus BLAISOUS Call da3 fin2 E ADHOCws_plus BLAISOUS bidon16 ad2 fout E ADHOCws_plus BLAISOUS bidon2 ad3 oper 0 a 1 000000 b 0 000000 c 0 000000 ke yword content options ARITHM3 3D input file name F1 with whole fin1 path 2D input file name F2 with whole fin2 path i 3D output file name F3 with whole out path oper type of the arithmetic operation 0 gt F3 F1 F2 A B 1 gt F3 A F1 B F2 C 2 gt F3 A F1 F2 B 3 gt F3 A F1 F2 B floating variable used in the p operation j floating variable used in the 7 operation lt floating variable used in the 7 operation Log book results Exce
369. sidy BTE Faso LULU CUT m aime MER ot ju inks TOLOI VUS UDC f il E CI Lanera adaga ju den ve fi a a 1 CDR CR 00 1 l vivem ine 100 2 AR meule sgr paio MH cut Viruslssten Sauset pee F Blink of 2D files If several images files are selected in the Parameters folder then new button box appear in the right button part of the image folder window File 1 File 2 File 6 depending of the files selected in the Parameters folder At the first display all these files are superimposed But if you click on a File n button you will display only one file at the same time Note that if you click on the Actualize full display button you will leave the blink mode and return automatically to the superposition mode During the blink you can let the position of the mouse unchanged and by the way see the differences of the zoom and of the zoomed pixel value For this don t move the mouse to click on the File n boxes the zoom position will change but use the shortcuts to select the blink files alt n alt 1 alt 2 alt 6 Comment or information boulesteix observatoire cnrs file CI ADHOCW HELP adw2d_c htm 4 of 5 15 02 02 09 33 50 ADw2D mixing different displays of images mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape
370. slice translations File structure information minimum and maximum Dumps files content modifications Macros and batches This program requests a 640 x 480 screen with 96 pixels per inch If your system doesn t offer such a screen a warning screen message will be displayed but you will nevertheless be able to run the program in a reduced display mode Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But file C ADHOCw HELP adwft htm 2 of 3 15 02 02 09 34 05 ADwFT File translator module the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwft htm Return to main ADHOCw menu file C ADHOCw HELP adwft htm 3 of 3 15 02 02 09 34 05 file Cl ADHOCw HELP adwft_a3 htm ADwFT Return to main ADHOCw help Return to main ADWFT help Getting observational data from VME Chile photon counting The format is the EIC compressed You can directly do a 3D gt 3D translation in the ADWET program from GHASP photon counting The format is ADA You must run the ADwT1 E01 function in order to build cubes with the photometric compensation and the suppression of the
371. ss Sepe Tst Gags peid 72 05 Crags Eppe Ts C6 kgs Eppe m atb ND th ha FP ekte Hikes ArNe Vila fab Tica y E EESTE E Hone r Jat mil Tad un lasite dites ris A n Is 1 Tso Sepe Tst Crags L peic Ts Gags Sped By this way it is very easy to superimpose up to 6 2D images For every 2D file the different parameters are Visualization mode not visible the file is not displayed square pixels the pixels appear to be square when zoomed smoothed pixels the pixels are smoothed when zoomed the square of the pixel disappears isophotes only isophotes are displayed pixels doesn t appear Square pixels isophotes isophotes are superimposed over square pixels smoothed pixels isophotes isophotes are superimposed over smoothed pixels Palette rainbow classical rainbow black and white inversed black and white color 1 other rainbow color 2 16 levels file C ADHOCw HELP adwa2d_c htm 2 of 5 15 02 02 09 33 50 ADw2D mixing different displays of images color 3 to discriminate large dynamics Threshold step overlapping The correspondence between the values of the image and the colors is obtained from 3 parameters the threshold lowest displayed value the step space between colors and the possible overlap If there is no scale overlap all the values larger than the last step are displayed like the last step If the scale overlap chec
372. ss color 16 possible colors Center cross thickness line width in screen pixels Center cross width symbol size in screen pixels Alpha delta epoch corresponding to the center position Text color for X and Y labels 16 possible colors Text size font size of the X and Y labels Text bold font of the X and Y labels can be bold or not Vertical and horizontal label spaces are defined separately Vertical and horizontal large tics space space between tics Large tics usually correspond to the labels Vertical and horizontal small tics space space between tics Small tics usually correspond to subdivisions Tics thickness in screen points Frame square can be drawn or not Frame color 16 possible colors Frame thickness in screen points Legend color 16 possible colors Legend text size font size for the legend Legend bold legend font can be bold or not Legend text free for the user file C ADHOCw HELP adw2d_o htm 3 of 6 15 02 02 09 34 23 Text and overlays Numerous features text or drawings can be inserted at any position For that press the swap to overlays button Tip freeze a screen coordinate by pressing the right mouse button This screen coordinate will be automatically set as default in the overlay dialog box For features with 2 coordinates rectangle ellipse freeze 2 successive coordinates This is a text file C ADHOCw HELP adw2d_o htm 4 of 6
373. st channels is a mixture with n 1 n 2 and n 3 Absorption if this checkbox is checked the highest channel values are taken instead of the lowest The operation is symmetric Substraction of lowest channels becomes substraction of highest channels and the channels values are ordered in decreasing mode n 1 means in this case the highest channel If the read value is null value it is not taken in account in the continuum reference and is also not changed no substraction occurs The input file can be of new ADHOCw type AD3 or old ADHOC type DA3 The output file is created as new ADHOCw type AD2 This function can use an execution mask When the execution mask doesn t allow the operation the channel value remains unchanged This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network file C ADHOCw HELP adwt1b13 htm 2 of 4 15 02 02 09 34 44 ADwT1 continuum substraction Macro definition Example SUBSTR_CONT fin E ADHOCws_plus BLAISOUS lambda ad3 fout E ADHOCws_plus BLAISOUS bidon ad3 oper 0 mode _emiss 0 keyword content options SUBSTR_CONT fins 3D input file name with whole path Pp fout 3D output file with whole path D OS oper type of operation 0 mean 3 lowest channels 1 lowest channel 2
374. t forget to save the ADC parameters Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adw2d_o htm Return to main ADHOCw menu Return to main ADw2D menu file C ADHOCw HELP adw2d_o htm 6 of 6 15 02 02 09 34 23 ADw2D kinematical functions ADw2D Return to main ADHOCw help Return to main ADw2D help Kinematical functions This function allows to get rotational curves and mass distribution from a radial velocity 2D file Important note selection of the pixels position angle in the classical case or position angle and radius in the extended case are done on p and 0 values which are sky coordinates p is the distance to the center of rotation and Bis the position angle drawings RV or RotV points individual pixels or crowns are using p and 6 values which are galactic coordinates p is the distance to the center of rotation and 6 is the position angle p and 6 are the polar coordinates in the plane of the galaxy p and 6 are the polar coordinates in the plane of the sky and 6 are angle with respect to t
375. taMI truc bmp Computation mode C Mo background Suppress background Bkadperchannel 0 PRESSE RTE D ee nes ey ale ei PT file CI ADHOCW HELP adwt1c11 htm 1 of 8 15 02 02 09 34 53 ADwT1 rough photometry Bkod per channel jo Store maero This function is supposed to compute the photometric corrections from zones profiles This function is only doing the analysis of the correction generating an ADX output ASCII file not the correction itself which must be done later function B15 This method of rough photometry takes only in account the total sum of profiles inside given areas to correct individual channel photometry This method is not so pure than the C11 function method The principle is the following the profiles are summed inside area which are defined in an ADZ input file Then the user gives or not a background value to suppress to the profile channels The correction Ax B which is written in the ADX output ASCII file is A 1 minimal_channel_ value and B 0 With this method it is possible to correct roughly from photometry variations when the more complex C05 function method Ax B based on the OH lines gives bad results The input 3D file must be not dephased original or simply corrected from cosmic rays The input ADZ zone file is an ASCII file containing the x1 y1 x2 y2 coordinates of the area to take in account The ADZ input file can easily be defined from the ADw3D zones function At the e
376. tar to analyze counted from 1 file C ADHOCw HELP adwt1_c 6 htm 2 of 7 15 02 02 09 34 48 ADwT1 seeing analysis box _ size of the analyzing square box Log book results Excepted the text of the macro and the ending execution message the following information is recorded 0210 01 Lower 09 23 seeing 2 256759 pixels 0210 01 Lower 09 23 seeing 1 954411 pixels 0210 01 Lower 09 23 seeing 2 523134 pixels 0210 01 Lower 09 23 seeing 2 256759 pixels 0210 O01 Lower 09 23 seeing 2 256759 pixel 0210 0l Lower 09 23 seeing 2 523134 pixel 0210 0Ol Lower 09 23 seeing 2 523134 pixel 0210 0l Lower 09 23 seeing 2 523134 pixel 0210 0Ol Lower 09 23 seeing 2 523134 pixel 0210 0l Lower 09 23 seeing 2 256759 pixel 0210 0l Lower 09 23 seeing 2 256759 pixel 0210 0Ol Lower 09 23 seeing 2 256759 pixel 0210 0Ol Lower 09 23 seeing 1 595770 pixel 0210 01 Lower 09 23 seeing 2 523134 pixels 0210 01 Lower 09 23 seeing 1 954411 pixels 0210 01 Lower 09 23 seeing 1 954411 pixels 0210 01 Lower 09 23 seeing 1 954411 pixels 0210 01 Lower 09 23 seeing 2 256759 pixels 0210 01 Lower 09 23 seeing 1 954411 pixels file C ADHOCw HELP adwt1_c 6 htm 3 of 7 15 02 02 09 34 48 Ch Ch Ch Ch Ch Ch Ch Ch Ch
377. tation scaling ADHOCw Ratation scaling XYZ translation and inversions far 2D ar ID tiles Input 2D or 3D file Output 2D or 3D file Choose file ene ee ASCII file containing the coordinates to superpose Simple shift 2 ESP Choose file C XY and or Z inversion C Rotation shift scale Shift x lo m fo Z fo Superposition of images or cubes Inversion inversion Y inversion Z inversion Rotation angle of rotation fo Center of rotation couneted from 1 e 257 00000 Yej257 00000 factor fi Substitution value 3 1 E 38 Load null into subst null is 3 1E 38 lt S Execute 7 Help x Abort EX Store macro The user must only notify the input 2D or 3D as well as the output 2D or 3D files The program recognizes file C ADHOCw HELP adwt1b11 htm 1 of 4 15 02 02 09 34 43 ADwT1 rotation scaling XYZ translations automatically the type of the input file The input file can be of new ADHOCw type AD2 or old ADHOC type DA2 The output file is created as new ADHOCw type AD2 You an choose simple shift only X Y and Z shifts are computed Shifts are float values inversion X Y and or Z dimensions are inverted rotation shift scale X Y and Z shifts rotation around a center of rotation units pixels numbered from 1 and scale enlargement factor are computed superposition of images or cubes the pixels in the original referential m and in the f
378. terference order will Step 2 initializing the 3D deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation deviation Step 3 buffering the writing zeros in the buffering spectra 1 20 buffering spectra 21 40 buffering spectra 41 60 ADwT1 PYTHEAS 1 547 0182 16 Batch Lower 18 16 47 G01 547 0182 16 Batch Lower 18 16 49 G01 547 0182 16 Batch Lower 18 16 51 G01 547 0182 16 Batch Lower 18 16 53 G01 547 0182 16 Batch Lower 18 16 55 G01 547 0182 16 Batch Lower 18 16 58 G01 547 0182 16 Batch Lower 18 16 59 G01 547 0182 16 Batch Lower 18 17 06 G01 547 0182 16 Batch Lower 18 17 09 G01 547 0182 16 Batch Lower 18 17 11 G01 547 0182 16 Batch Lower 18 17 12 G01 547 0182 16 Batch Lower 18 17 14 G01 547 0182 16 Batch Lower 18 17 16 G01 547 0182 16 Batch Lower 18 17 18 G01 547 0182 16 Batch Lower 18 17 20 G01 547 0182 16 Batch Lower 18 17 22 G01 547 0182 16 Batch Lower 18 17 23 G01 547 0182 16 Batch Lower 18 17 25 G01 547 0182 16 Batch Lower 18 17 26 G01 547 0182 16 Batch Lower 18 17 27 G01 547 0182 16 Batch Lower 18 17 29 G01 547 PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS CUBE Info PYTHEAS_ CUBE Info PYTHEAS CUBE Info PYTH
379. terpolated in the case of the micro phase correction Nevertheless if the beam is large gt 5x5 pixels the user can try to check the box and could obtain other results The input 3D file must be not dephased original or simply corrected from cosmic rays The input phase file is the parabolic phase see ADHOCw function C01 The input ADZ zone file is an ASCII file containing the x1 y1 x2 y2 coordinates of the area to take in account The ADZ input file can easily be defined from the ADw3D zones function At the end the coordinates are rearranged in order to have x2 gt x1 and y2 gt y1 but the original file is not changed The ADZ zones file is compatible with the old ADHOC DOS area files functions 13 and 48 The only change is that the coordinates can be now float and not limited to integers 0 or 999 values are not taken in account as well that comment lines at the end For instance the following file which is coming from an old ADHOC sequence is valid 35 23 245 101 Zone J 280 353 532 475 Zone 2 4 175 500 207 Zone 5 5 249 302 351 Zone 7 143 313 241 389 Zone 9 143 453 143 453 Zone 11 0 00 0 Zone 3 0 00 0 Zone 4 0 00 0 Zone 6 file C ADHOCw HELP adwt1_c5 htm 3 of 11 15 02 02 09 34 46 ADwT1 photometry from OH 0 Zone 8 0 Zone 10 999 999 999 999 Zone 0 zones Possible input for numerous ADHOC functions 0 0 0 0 0 0 9 but new files as the following are also vali
380. th the mouse approach the summit of a channel value The cursor normally a cross will change to a double vertical arrow In this case by dragging pressing permanently the left button of the mouse the user can change the value and the shape of the profile The graph will be redrawn when the left mouse button will return to the upper position The modified value is always red current value The origin value is gray Replace 3D profile in the 4D3 file Channel original value and modified value are only current values at the mouse location Graph channel limits allows a possible zoom in X file C ADHOCw HELP adw2d_e htm 6 of 8 15 02 02 09 33 54 ADw2D 3D profiles Full Y scale if checked the graph mini and graph maxi are automatically computed If not checked the user can define the Y scale of the drawing Redraw with parameters above must be pressed if the Y scale are changed by the user Store 1D profile RV to AD1 stores onto disk the values of the profile in the AD1 format X is the radial velocity Y is the intensity Store 1D profile lambda to AD1 stores onto disk the values of the profile in the AD1 format X is the wavelength Y is the intensity Store 1D profile channels to AD1 stores onto disk the values of the profile in the AD1 format X is the channel Y is the intensity Print window print the whole ADw2D profile window Save graph to BMP file saves the graph area to a BMP graph f
381. that the full directory folder name must be extracted in order to put correctly the files in the ADHOCW and ADHOCW HELP directories See at the end of this text the different files expected in the different directories at the end of the decompression 2 As the ADHOCW EXE program is the unique entry of the software add the ADHOCw program to the start menu click on the START icon on the bottom toolbar with the RIGHT mouse button select OPEN a window opens select PROGRAMS a new window opens select FILE NEW SHORTCUT browse and select ADHOCw ADHOCw exe Continue as next give ADHOCw as shortcut name TERMINATE Now ADHOCw program is included in your START menu You can also add the ADHOCw program to the dekstop the process is similar click with the RIGHT mouse button on the background deskstop screen select NEW SHORTCUT browse as above The ADHOCw program will be also visible on your dekstop file C ADHOCw HELP adw_inst htm 1 of 3 15 02 02 09 35 06 ADHOCw software installation 3 help un ADHOCw and click immediately on the new users button to get a full 4 inform J BOULESTEIX boulesteix observatoire cnrs mrs fr of your ADHOC use and possible difficulties Request to be recorded on the ADHOCw user list i
382. the color and the scale begins again from the bottom when the maximum color is reached To change the step or the threshold there are two ways click on the adequate button or fixed values or edit yourself the step or threshold field Then click on actualize full display Zoom area and pixel position value On the top of the screen the left image usually represents the 19x19 pixel zoom of the mouse position On the right the values of the XY position and the value of the image pixel are displayed You can change the cursor size default 1x1 pixel in this case the pixel content will be the mean value of all the pixels included in the enlarged cursor Compute sum again the sum of the interferograms or of the wavelength maps is computed and displayed A scrolling box allows to choose the 3D memory to sum interferograms or wavelength maps Display 1 channel you can display one given channel of the interferograms or of the wavelength maps A scrolling box allows to choose the 3D memory to use interferograms or wavelength maps An edit box allows to define the number of the channel numbered from 1 Display channel movie you can display a channel movie of the interferograms or the wavelength maps A scrolling box allows to choose the 3D memory to use interferograms or wavelength maps You can stop on a channel display the previous one or the next one and change the movie speed file C ADHOCw HELP adw3d_b htm 2 of 3 1
383. the macro file Present macro PHASE fin D ADHOCws_plus BLAISOUS Cal1 da3 ph_bru D ADHOCws_plus BLAISOUS Phas_bru AD2 ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 sum_cal D ADHOCws_plus BLAISOUS Sum_cal AD2 cal ru D ADHOCwS _plus BLAISOUS Cal RV AD2 x1 6560 000000 x sppendiandisave OVER White and sme Save ifi emea a uit file C ADHOCw HELP adwt1_ba htm 1 of 6 15 02 02 09 34 07 ADwT1 batchs You must first indicate the file containing the macros ADM type If the file doesn t exist it will be created If the file already exists its content will be displayed in the Present content of the macro file box You can then Overwrite and save clean the file and put your unique macro or Append and save add the last macro command to the content of the ADM file ADHOCw Recording a macro File containing the macros ADM DADHOCws_plus BLAISOUStoto adm Present content of the macro file SUM3D2D fin D ADHOCwSs_plus BLAISOUS Oba da3 fout D ADHOCws_plus BLAISOUS toto ad 2 SMOOTHSY fin D ADHOCws_plus BLAISOUS Oba da3 fout D ADHOCws_plus BLAISOUS toto2 ad3 square 3 You can edit the macro file if needed it and then save it Present macro PHASE fin D ADHOCws_plus BLAISOUS Cal1 da3 ph_bru D ADHOCws_plus BLAISOUS Phas_bru AD2 ph_prb D ADHOCws_plus BLAISOUS Phas_prb AD2 sum_cal D ADHOCws_plus BLAISOUS Sum_cal AD2 cal re D ADHOCwS _plus BLAISOUS Cal _ RV AD2 x11 6560 0000
384. the pupil is enlarge on the spectrum itself This option is recommended The program takes a pupil width which is h 3 2 pixels his here the height of one individual spectrum from F01 A matrix grid with weight is used to integrate in X and Y on the base of weight 10 x_dist 2 10 y_dist 2 where x_dist and y_dist are in pixels of the observation files If the box is not checked the spectrum is nevertheless integrated but only in Y with a weight in Y which is equal to 10 y_dist 2 Reference object line this value is set in the new ADP file in order to compute velocities from the wavelength cube It is the zero wavelength of the object 5 Result Output 3D wavelength file as the output cube will have different dimensions the output cube will take place in a new directory as well as a new ADP parameter file In this case a special window creating output cubes with different dimensions will appear Output ADP parameter file this file will be created in the same directory than the output 3D wavelength file Output TXT verification file zero wavelength calibration interference order this file records the channel number of the first calibration line of individual micro lenses Variation in these values indicates a bad tuning of the interferometer The output format is Zero wavelength verification file numlens ixl iyl ix2 iy2 channel 0 221 3 292 7 26 667 1 339 3 410 7 26 704 2 457 3 530 7 25 365 5
385. the residual doing the P computation for the next passes If you underestimate the P factor there is no real importance and can be even recommended if you compensate at the next pass and at the end you substract all the residuals For example suppose that the photon number measure above background of the OH line is 100 pixel At the first pass you will use a substraction factor which will be at maximum P1 1 1 sqrt 100 0 9 At the second pass the residual will be 100 1 0 9 10 photons pixel and P2 1 1 sqrt 10 0 68 At the third pass the residual will be 10 1 0 68 3 2 photons pixel and P3 1 1 sqrt 3 2 0 44 But as we allow only 3 passes P3 will be enforced to 1 in order to suppress all residuals At this step the OH substraction will be negligible Note that the computation of P is more complex if spatial or spectral smoothings occurred before In fact the smoothing changes the noise for example if you have done a spatial rectangular XY smoothing of 5x5 nx ny 3 and a spectral Z smoothing of 3 nz 1 the noise will be diminished of a factor 5 for the spatial smoothing and of a factor sqrt 3 for the spectral smoothing So P1 1 1 sqrt 100 25 3 0 988 and P2 will have a similar computation P2 1 1 sqrt r sidu 25 3 As P n lt P n 1 the computation has no convergence and the OH substraction is more difficult wnen the number of passes increases Nevertheless the residuals are quickly negligible Comment or in
386. tm 2 of 2 15 02 02 09 34 04 ADwET File translator module ADwFT ADHOCw program to translate 2D and 3D files Return to main ADHOCw help How to transfer observational data ae scale 410 ADHOCw File Translator sson100 Jex ppe PICTTELIEEEEEEENEE EEE EEE TELEEEEES Jad 30 2D gt 20 3D gt 2D slices 2D slices gt 30 File parameters Dump and modify Macros Presentation of the ADHOCw File Translator The ADHOCw Fille Translator allows to convert 2D and 3D files It reads and writes various data formats ADHOC FITS IDL and others If you ignore the type of a file use the File_parameters function to get the information 3D gt 3D converts a 3D files ordered by spectra or ordered by channels 2D gt 20 converts a 2D file 3D gt 2D slices converts a 3D into a set of 2D files 2D slices gt 3D converts a set of 2D files into a 3D file File_parameters gets the file type allows to modify its parameters and gets mini amp maxi n data values ADHOCw Dump and modify give a direct reading and writing access to the data Macros are automatic batchs to convert sequentially several files Analyse et Note ADHOCw input files for data reduction are limited to D pouillement OCw new formats default extension AD2 and 4D3 Homog ne des old S DHOC YISU2 ISUS formats integers16 extension DA2 and D43 Observations 2D or 3D F
387. ton files CIG or TRI files C Deferred acquisition from CCD FITS acquisition FIT files frosoxs14 7 interlacing 2 7 X Abort Help You can read or integrate easily cubes This cubes will stay in the RAM memory this program needs a large available memory If you integrate IPCS acquisition or deferred FITS acquisition the program will first read and display all the ADA TRIM or FITS files using for that a background task If you read AD3 or DAS cubes the cubes are just read before display Important note for users the easiest way to get quickly the best display in ADW2D and ADw3D programs is to use the zoom and unzoom facilities in any image folder To zoom x2 simply move inside the display the mouse at the pixel that will be located in the center of the new display area and press the right mouse button To unzoom 2 simply move inside the display the mouse at the pixel that will be located in the center of the new display area and press the right mouse button while pressing the shift key file C ADHOCw HELP adw3d htm 1 of 2 15 02 02 09 33 57 ADw3D 3D display module Acquisition modes for the basic cube General functions Main 3D display screen Main 2D display screen Defining profile zones in the 2D image Loading phase Getting wavelength maps Getting monochromatic continuum and radial velocities maps This program requests a minimum screen of 1280x1024 wit
388. tware installation Running ADHOCw The ADHOCw files and suffixes Conventions null values coordinates Shared files and network access ADHOCw HTML help Assigning file extensions for direct execution Description of the programs The ADw2D program display of 2D images The ADw3D program display of 3D cubes The ADwT1 program data reduction file C ADHOCw HELP adhoew htm 1 of 2 15 02 02 09 33 43 ADHOCw software for Windows 32 bits The ADwFT program 2D and 3D data file translation The ADwIPCS program photon counting real time acquisition Getting data From VME Chile photon counting From GHASP photon counting From CFHT CCD From Byurakan CCD From SAO photon counting Reduction procedures A typical procedure for CCD data or photon counting CIGALE data A typical procedure to reduce TIGER and or PYTHEAS data User manual How to print your own copy of the User Manual Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adhocw htm file C ADHOCw HELP adhoew htm 2 of
389. ults indicates the additional tilt angle and its declination into millimeters relative to a filter diameter file C ADHOCw HELP adwt1_h8 htm 4 of 6 15 02 02 09 35 02 ADwT1 Interference filters Log book results None Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special file C ADHOCw HELP adwt1_h8 htm 5 of 6 15 02 02 09 35 02 ADwT1 Interference filters printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_h8 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_h8 htm 6 of 6 15 02 02 09 35 02 ADwT1 Perot Fabry talons ADwT1 Return to main ADHOCw help Return to main ADwT1 help H09 Perot Fabry etalons characteristics and Queensgate constants PF characteristics and Queensgate constants are regularly updated in successive ADHOCw versions ADHOCW Perot Fabry talons characteristics and Queensgate constants E Perot Fabry talon list Selected PF characteristics Interference order fi 938 Se Gls cs at wavelength 4 6562 780 Print window Drawing scales Save graph to BMP Lambda mi
390. unique covering all the galaxy Theses options are accessible by clicking on the Params r button The left part of the general display window appears like this file C ADHOCw HELP adw2d_k2 htm 1 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns Defining the crown sectors Then if the user clicks on the Edit a params r array button the following window will appear file C ADHOCw HELP adw2d_k2 htm 2 of 12 15 02 02 09 34 27 ADw2D kinematical functions user made crowns AN ADw2D ADV edition _ Of x ADw2D ADV array for velocity curves Create a regular array with following parameters Crowns pixels 20 Systemic velocity Km s 2320 00 This option gives the possibility to fill a large number PA w t top degrees 36 00 Inclination w r sky degrees 30 00 of cells before modifying them manually Half sector degrees 20 00 R min pixels E 28 00 R max pixels 128 00 Load array from ADVY file Suppress line gt fo o Save array as ADV file Insert a new line BEFORE line gt 1 Clear array Help ADY file is ASCII and printable Acquire array amp go to image Quit whithout reading array Notes 1 Rmin and Rmax are in pixels on the sky PAmin and PAmax are in degrees with respect to the top of the image and counted in direct sense inverse clockwise Ys is in km s incli is in degrees with respect to the sky plane
391. uppress a continuum in every pixel but independently each one se ADw continuum Input 30 file Output 32 file _ Choose file i Substraction of the mean of the 3 lowest channels Substraction of the lowest channel Substraction of the mean of all channels Substraction of the channel 4n 1 lowest lz highest n f Absorption M Use an execution mask J execute _ 7 wep X abort Store macro The user gives the input and output 3D files file C ADHOCw HELP adwt1b13 htm 1 of 4 15 02 02 09 34 44 ADwT1 continuum substraction Substraction of the mean of the 3 lowest channels the mean of the 3 lowest channels is computed and substracted from all the channel values This can give negative results but the operation is not so sensitive to the noise of the channels Substraction of the lowest channel the lowest channel value is substracted from all the channel values The lowest channel becomes 0 Substraction of the mean of all channels half of the channel values will become negative Substraction of the channel n in the lowest order the channel values are first ordered in increasing mode If n 4 for instance this means that the channel which is in the lowest but not the lowest really only the 4th in the order of the lowest will be substracted If n 1 the operation is similar with the substraction of the lowest channel The substraction of the mean of the 3 lowe
392. ut the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1 htm Return to main ADHOCw menu file CI ADHOCW HELP adwt1 htm 2 of 2 15 02 02 09 33 46 ADwT1_gene ADwT1 Return to main ADHOCw help Return to main ADwT1 help Generalities When you execute the ADwT1 program of the ADHOC software the first screen is the following ADHOCw beginning ADwT 1 Version 2000D JBx Obs Marseille Cw data processing softwar The ADHOC 3D software has beer developped at Marseille 5 Observatory lt can be used for data obtained with CIGALE TIGER or PYTHEAS instruments 30 data are images in which pixels are spectra ADHOCw manages the windows network NetBEUI or others All files data and executables can be access through the network All the files are shared wher read This means that different tasks can access simultaneously to common input files Data Null values are accepted An ADHOCw parameter file type ADP is required t define the main 3D parameters and the default directory All the data files of this directory are supposed to have the same and Z dimensions ADHOCw AS AAE SA EE PR iee SAA HAS EAA SE ERLE IRL ete te ie CRSP Cee AA ERS tes tee ies Anal t Open an existing ADHO
393. v Moeaa Display channel movie Y Interferograms Interferograms v Save 2D image Load 2D image Effect when clicking left button of the mouse Define profile zones inversed C Scale max 2240 C Threshold 0 Load 11 zones from ADZ file 4 1 10 10 100 100 1000 1000 Step Xe 2 140 Mini 107 000000 Maxi 11869 000000 2 Profile displayed in zoom or image 1 None v 10 10 Semen of profiles 100 100 Square in pixels 000 1000 Normalization Scale min 0 individual S Drew profiles D Scale overlap Continuum normal v file C ADHOCw HELP adw3d_2t htm 1 of 2 15 02 02 09 34 13 ADw3D full size main 2D file CI ADHOCW HELP adw3d_2t htm 2 of 2 15 02 02 09 34 13 ADw3D full size ADw3D_E AD ADHO ne 20 AVL A Cube dimensions Ix 1512 y 1512 le 127 Mouse profile area i 1 pix v By Printer setup B Print screen aa Save data Help 1 a Waiting gap sec X Quit the program Y Value Taam 1019 nivale General Statistics Phase Sum Interferograms Wavelength maps Mono cont RY 1 94 100 159 153 6 134 400 201 439 393 418 415 455 channel 14 93 10 383 170 443 201 8 394 419 416 456 Active the real time sum of interferograms Compute sum again Display a channel 1 a intert v Display channel movie Interferograms X Interferograms v Save 20 image Effect when
394. ve with a width given in floating pixels Values lt 1 of the maximum are considered to be 0 in order to minimize matrix size Lorentzian mode is a lorentzian curve with a width given in floating pixels Values lt 1 of the maximum are considered to be 0 in order to minimize matrix size Smoothing mode are predefined patterns values are displayed on the right Smooth Smooth Blur Sharpen Detail Edge enhance Edge enhance User smoothing mode is a pattern which is pre defined by the user and cans be simply loaded from an ASCII file special ASCII format The user can edit any of the patterns even the predefined ones and store them as user patterns in ASCII code in order to use them later as user smoothing patterns The user must define the names of the 2D or 3D input and output files The type of the input files 2D or 3D is automatically recognized The null values are not taken in account in this computation The input file can be of new ADHOCw type AD2 AD3 or old ADHOC type DA2 DA3 The output file is created as new ADHOCw type AD2 AD3 This function can use an execution mask This function can be execute directly by pressing the Execute button or in batch by pressing the store macro button The data files can be shared beween several process or users and can be located on other computers accessible on the network User file containing filter values file C ADHOCw HELP adwt1_b9 htm 3
395. w ADP file lF pou do this T the history log file ADL will also change name same name as ADP the command numbering will begin at zero again ag Confirm change Cancel save file C ADHOCw HELP adwt1_a1 htm 3 of 4 15 02 02 09 34 19 ADwT1 Basic 3D parameters It is not simple for the user to change path for the new ADP file It is suggested to quit ADHOCw to copy the ADP file in another directory changing its name inside the new directory is suggested and to run ADHOCw again in the new directory as suggested in the dialog box which appears if the user wants to write an ADP parameter file in another directory ADw warning parameter file lt is impossible to write a new parameter file ADP in a different directory because the ADP file indicates the default di irector Solution write the new ADP file ir the default directory quit ADHOCW copy the ADP filein the new director un ADHOCw and request at beginning the nEw ADP parameter file yf Continue Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape lExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located on the adhocw help adhocw htm file This file is adwt
396. w HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_b5 htm Return to main ADHOCw menu Return to main ADwT1 menu file C ADHOCw HELP adwt1_b5 htm 4 of 4 15 02 02 09 34 39 ADwT1 masking operations ADwT1 Return to main ADHOCw help Return to main ADwT1 help B06 Arithmetic and masking operations between 2D or 3D files ED ADw 3D arithm2 ADHOCw ALHAMG HC Ghd asking GOSSES feiwees twa PL ar SERIES Input 2D or 3D file F1 Coase TE CoE Input 20 or SD file F2 Choose file To Output 2D or 30 file FS Choose file O Anthmetic operation Value of A i F3 A F1 F2 B FS 4 F1 IF2 B Set A to minimum null F3 maximum of F1 and F2 Set to maximum F3 minimum of F1 and F4 null not takeni F3 pull if F2 is null value F1 else Val pp F3 pull if F2 is null value F2 else US F3 F1 if F2 is inside 4 and B values null else lo F3 F1 if F2 is outside 4 and B values null else F3 F1 if F2 is inside A and B values F2 else Set B to minimum null F3 F1 if F2 is outside 4 and B values F2 else Set B to maxinum F3 F2 if F2 is inside 4 and B values F1 else F3 F2 if F2is outside 4 and B values F1 else file C ADHOCw HELP adwt1_b6 htm 1 of 5 15 02 02 09 34 39
397. w htm file This file is adwscr htm Return to main ADHOCw help Return to main ADw2D help Return to main ADw3D help Return to main ADwT1 help file C ADHOCw HELP adw_scr htm 3 of 4 15 02 02 09 33 47 ADw screen warning Return to main ADWFT help Return to main ADWIPCS help file C ADHOCw HELP adw_scr htm 4 of 4 15 02 02 09 33 47 ADw2D 2D display module ADw2D ADHOCw program to display 2D files allows also to superimpose 3D profiles Return to main ADHOCw help AR ADHOCw 2D display ojx J Boulesteix ADHOCw 2D display C Open a context file ADC previous display parameters Peseneesnnhonyspecwsnseasessg het LE PE ETES ENT senses ET TE ENT EE EEE ET PEN TEE ET ENT ES EST EEE TENTE EL LI OLLEEN EEE L PEEIT TEL SES EE DEEE EEE REEET EEE This program can directly read FITS files file C ADHOCw HELP adw2d htm 1 of 3 15 02 02 09 33 47 ADw2D 2D display module Important note for users the easiest way to get quickly the best display in ADW2D and ADw3D programs is to use the zoom and unzoom facilities in any image folder To zoom x2 simply move inside the display the mouse at the pixel that will be located in the center of the new display area and press the right mouse button To unzoom 2 simply move inside the display the mouse at the pixel that will be located in the center of the new display area and press the right mouse button while pressing the Shift key
398. wo pages folders Image which is the display and Parameters which are the different files file C ADHOCw HELP adwa2d_b htm 1 of 3 15 02 02 09 33 48 ADw2D main display screen ZOOM The image area can be easily zoomed The simplest way is to click on the right button on the mouse it will be a zoom x 2 centered at the mouse location Similarly you can unzoom of a factor 2 by clicking on the right button of the mouse but pressing at the same time the shift key Another way is to change the Image area box which gives the size of the displayed image Field You can move the field simply by dragging the white square in the small full image area located on the top at right You can also change the X0 and YO values A third way is to use the scroll bars around the image Palette You can change the color palette different rainbows black and white color inversions user palette User palette allows the user to define himself the colors Step threshold and scale overlap The correspondence between the values of the image and the colors is obtained from 3 parameters the threshold lowest displayed value the step space between colors and the possible overlap If there is no scale overlap all the values larger than the last step are displayed like the last step If the scale overlap checkbox is checked there is a modulo to compute the color and the scale begins again from the bottom when the maximum color is reached
399. xplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adhocw help adhocw htm file This file is adwt1_ge htm Return to main ADHOCw menu Return to main ADWT1 menu file C ADHOCw HELP adwt1_ge htm 3 of 3 15 02 02 09 33 46 ADw screen warning ADHOCw Return to main ADHOCw help Return to main ADw2D help Return to main ADw3D help Return to main ADwT1 help Return to main ADWFT help Return to main ADWIPCS help Warning display message file C ADHOCw HELP adw_scr htm 1 of 4 15 02 02 09 33 47 ADw screen warning Te warning Oe x Warning Your windows screen is not optimal for ADw3D Ideal size is 1280 x 1024 Not OK Yours is only 1024 x 768 Not Q Ideal Pixel per Inch value is 96 OK Yours is OK 96 But you can work nevertheless like this If the screen size is smaller than required you will need to use the windows scroll bars to access to the whole window IF the Pixel per Inch value is not 96 the best is to change it nous if not the graphics and the test could be largely distored sometimes unreadible To change the Fisel Per Inch value go to the Control Fannel and then to the Display tone of the Window system Put the fonts to small fonts instead of lange fonts Continue execution x Quit the program now Such a window appears when you launch the programs ADw2D ADw3
400. y to postpone an execution into a batch For this look to the section batches Help which is a complete HTML help branching instantaneously to the detailed help of the displayed function Hide task manager window allows to hide temporarily the task manager window This cannot be done on the task manager window itself which has no minimizing icon Then a button Show task manager window will replace the Hide task manager window on the function menu window Bring task manager to front allows to switch to the task manager window The global logbook area is the logbook mixing all the messages of the functions running during the present ADwT1 session All the session logbooks are also copied append into a grand global logbook an ADL ASCII file To look back to the logbook relative to previous sessions you must access yourself to the ADL ASCII file which is the memory of the whole treatment since the creation of the ADP parameter file The ADL and ADP files have the same name an MY_OBS ADP parameter file will create a MY_OBS ADL log file Comment or information boulesteix observatoire cnrs mrs fr Note all ADHOCw help is in HTML The present HTML browser is a very simple browser incorporated to ADHOC But the ADHOCw HTML help can be directly accessible to your favorite HTML browser Netscape IExplorer for extended operations extraction of text or images special printings The ADHOCw HTML help is located in the adho
401. ymbo Frame Symbols Digits Legend amp add Superimpose usually when redrawing the graph the graph is first cleared If this box is checked it is possible to superimpose several successive graphs several different polynomial curves for example No axis usually the zero V axis 0 km s in case of RotV systemic velocity otherwise and the r 0 line are drawn in dash style If this box is checked the zero axis are not drawn V R axis legend the RV or RotV text Y axis is not drawn if this box is not checked Km s pix legend the r text X axis is not drawn if this box is not checked Line width width of the outside line of the frame in screen points Axis fonts for publication axis fonts are totally parametrable Frame Symbols Digits Legend amp add Digits fonts for publication digits fonts are totally parametrable file C ADHOCw HELP adwa2d_k1 htm 5 of 10 15 02 02 09 34 26 ADw2D kinematical functions full graph Offset for axis digits in order to get a perfect graph X axis and Y axis labels can be slightly shifted in X of Y Offset values are in screen points Frame Symbols Digits Legend amp add Add TXT curves Legend text the user can write a legend at a given location in the graph If the text string is null no text s written Legend X and Y these are the coordinates of the text of the legend in screen points Legend fonts for publication legend fonts ar

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