Program for masking `hot spots` on CCD data (C) SAO AS USSR VLVSoft 1991 Usage : COSMETIC.EXE [-x sizex] [-y sizey] [namein] [nameout] [maskname] where sizex - size of input image along X-direction( default= 512) sizey - size of input image along Y-direction( default= 512) namein - name of input file nameout - name of output result file maskname - name of text file with masks of 'hot spots' and defects
COSPAR
Program for analysing cosmic hits on CCD data (C) SAO Russian AS VLVSoft 1993 Usage : COSPAR.EXE [-x sizex][-y sizey][namein1][namein2][maskname][-d dev] where sizex - size of input image along X-direction( default= 530) dev - deviation parameter ( default - from console) sizey - size of input image along Y-direction( default= 580) namein1 - name of input file N1 namein2 - name of input file N2 maskname - name of result file with mask of hits
CREATSP
Program for creating of image with spectra' strobes (C) SAO Russian AS,Marseille Observatory VLVSoft v.01 18-11-1994 Usage : CREATSP.EXE [-w wid] [-x sizex] [-y sizey] [filgeo] where filgeo - name of text file with coefficients of polynoms (default name - geometry.exa) sizex,sizey - size of result image on both coordinates (default = 530 580) wid - width of modelled spetra ( by default = sigma*3.0)
CVIZ
Program for CIGALE/TIGER/PYTHEAS data cubes managing and processing (C) SAO Russian AS VLVSoft v.1.03 08-02-95 Usage : CVIZ.EXE [-e] [-s] [-w wmin wmax] [-x xleft xright] [-y ytop ybot] [-r][-f widfact][-d][-a][-c contnam][name1][name2][...nameN] where wmin,wmax - limits of argument for all profiles xleft,xright,ytop,ybot - leftmost,rightmost,upper and lower showed profiles name1,name2,...nameN - name of files with data cubes contnam - name of cube with continuum values widfact - factor of component widths transform (default = 1) Key -e indicates on work in EGA-mode with VGA adapter Key -s suggests fixed order of components (as set in GAUSAN.EXE) Key -r provides automatical restoring of last approximation in GAUSAN Key -d provides using of variable doublet parameters in GAUSAN Key -a provides quiet mode for wavelength in GAUSAN
FVIZ
Program for image vizualization and some processing (C) SAO Russian AS VLVSoft v.05 27-01-95 Usage : FVIZ.EXE [-e] [-w] [-f|l] [-x Xcen] [-y Xcen] [-s Scale] [-n|N] [-h hdlen][-m][-p Numpal][-t Twait][name1] [name2]... where Xcen,Ycen,Scale - coordinates of center and scale for image fragment hdlen - length of image file header (default=0) name1 - name of file with image name2,..- names of next workfiles(default - no) Numpal - number of palette will be used by default Twait - time of waiting for any user's action (default - no) Key -e indicates on work in EGA-mode with VGA adapter Key -w permits writing to image file Keys -f & -l indicate on output first or last image fragment Keys -n and -N allow output symbol data while repers coordinates re-reading from disk file Key -m provides definition of color level even service file exists
GAUEXT
Program for gaussian spectra extraction from detector frame (C) SAO Russian AS VLVSoft v.02 09-02-1995 Usage: GAUEXT.EXE [-b left right] [-n numsp]inpimage resfile [filgeo] [-d] [-y shiftY][-w AddWid] where left,right - borders for integrating (default = 5 MX-0) numsp - amount of adjacent spectra ( default = 3) inpimage - name of file with input image filgeo - file with spectra' geometrical params(default - geometry.exa) resfile - file with result spectra shiftY - shift of extration zone on Y (default = 0) AddWid - additional part into spectra width ( default = 0.0) Key -d using for producing of additional information
GEOPREP
Program for preparing of geometry data for bidimensional spectra (C) SAO Russian AS,KPNO,Marseille VLVSoft v.02 1993 Usage: GEOPREP.EXE [-f] [-r numrep] [-p power] [-x sizex] [-y sizey] [-nosort] [filgeo] [filpos] [filnum] [geores] where filgeo - name of text file with repers' coordinates filpos - name of text file with measured position of individual spectra filnum - name of text file with associated numbers of spectra geores - name of file with result : coefficients for each spectrum (default - geometry.pol) numrep - amount of repers in one line of repers' grid (default = 7) power - power of approximating bidimensional polynom (default = 3) sizex,sizey - size of result image on both coordinates (default = 512 512) Using of key -nosort prevents sorting of input file with repers' coordinates Key -f provides writing additional data to file geometry.tmp Using -F produce additonal image file strobe.dat (512 by 512 px) with predicted spectra' position
GAUSAN
Program for Gauss-decomposition of vector data (C) SAO Russian AS VLVSoft v.04 10-02-1995 Usage : GAUSAN.EXE [-x xmin xmax] [-w wave0] [-d dist relamp relwid] [-e] [-r] [-f widfact] [-a] [-F] filnam where xmin,xmax - min&max argument values (default - from file *.PAR) wave0 - restframe wavelength dist,relamp,relwid - distance and relations for doublet's components widfact - factor of width transform while it restoring filnam - name of input file Key -e indicates on using EGA-mode (default - VGA) Using of key -r provide restoring of parameters from gaus_sol.res Using of key -D instead of -d provides FIXED values for doublets ! The same for key -F : first entered parameters will be used everythere Using of key -a allows to avoid question about rest wavelength
IMAR
Program for image arithmetics (C) SAO Russian AS VLVSoft 18-11-1994 Usage: IMAR.EXE [operation] [filnam1] [filnam2] [filnam3] [const1] [const2] [const3] where operation - (+,-,/,*,-lg,-ln) filnam1 - name of input image 1 filnam2 - name of input image 2 filnam3 - name of output image const1,const2,const3 - constants for calculation Size of output image equals size of original
LINID
(C) SAO Russian AS VLVSoft v.05 24-01-1995 Usage: LINID.EXE [-p pow][-l len][-w wid][-d|-D disp][-a][-s][-f][-z] [-e][-m maskfil][-y min max][-c filcoef] [compspec lintab] [inspec outspec] where pow - power of dispersion approximating polynom(max=6) (default=2) len - length of input spectrum ( default - from file) wid - width of instrumental profile(default=5) min,max - limits for comparison spectrum respresentation filcoef - file with coefficients channels = > wavelength compspec - name of file with comparison spectrum lintab - table of spectral lines wavelength inspec - input spectrum to be linearized outspec - result of linearization maskfil - file with lines' positions Key -d indicates on input value of dispersion by user When key -D is using, necessary set dispersion value(in A/pix) Key -a executes automatic procedure with lines` mask and wavelength from lintab Key -f provides precise background estimating in each line centering Key -s indicates on using details in object`s spectrum in forming disp.curve only in manual program mode Key -z provides using same values (x0,dx,step) for all linearizes data When key -c is applying, comspec & lintab must be omitted
PRFTEST
Program for spectra parameters determination over detector frame (C) SAO Russian AS VLVSoft v.02 09-01-1995 Usage : PRFTEST.EXE [-w width][-b left right] [-n numsp] inpimage [filgeo][-d][-a AmpLim][-y YcrdLim][-f FWHMLim][-p power] where width - height of integration aperture(default=5,<30) left,right - borders for integrating (default = 10 MX-0) numsp - amount of adjacent spectra ( default = 3) inpimage - name of file with input image filgeo - file with spectra' geometrical params(default - geometry.pol) AmpLim, YcrdLim, FWHMLim - limits for max.variation of profile params by defaults - 0.9 1.0 0.5 power - order of approximating polynoms ( default - 3) Using of key -d provides extended output of results
PRFTESTO
Program for spectra parameters determination over detector frame (C) SAO Russian AS VLVSoft v.03 08-02-1995 Usage: PRFTESTO.EXE [-w width][-b left right] [-n numsp][-p Numfrag]inpimage [filgeo][-a AmpLim][-y YcrdLim][-f FWHMLim] where width - height of integration aperture(default=5,<30) left,right - borders for integrating (default = 5 MX-0) numsp - amount of adjacent spectra ( default = 3) Numfrag - number of fragments for spectra dividing (default = 21) inpimage - name of file with input image filgeo - file with spectra' geometrical params(default - geometry.pol) AmpLim, YcrdLim, FWHMLim - limits for max.variation of profile params by defaults - 1.00 0.50 0.75
SPEXTR
Program for spectra extraction from detector frame (C) SAO Russian AS VLVSoft v.02 1993 Usage: SPEXTR.EXE [-w width][-b left right][-s SlitStep] [inpimage][resfile][filgeo] where width - height of integration aperture(default=5,<100) left,right - borders for integrating (default = 20 MX-0) SlitStep - step for slit function producing (default = 1) inpimage - name of file with input image filgeo - file with spectra' geometrical params(default - geometry.pol) resfile - file with result spectra
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