SIMPLE = T / LONG-SLIT DATA REDUCTION R_DIR = 'e:\obs\s060927\' / DIRECTORY FOR READING DATA W_DIR = 'E:\obs\work\for_Zasov\n7457\sunsky\' / DIRECTORY FOR WRITING DATA NIGHT = S400 / NUMBER OBSERVING NIGHT CCD_CUT = '22,1,2066,1024' / REGION WITHOUT OVERSCAN (X0,Y0,X1,Y1) CUB_OBJ = '11' CUB_STAR= '02' CUB_NEON= '05' CUB_FLAT= '11' OBJ = '01,02,03,04' / NUMBERS OBJECT FILES FLAT = '06,07' / NUMBERS FLAT FILES NEON = '6,14,19' / NUMBERS COMPARISON SPECTRUM FILES STAR = '04,05' / NUMBERS STAR FILES OBJ_XSHI= 1 / ENABLE SHIFT along X OFFSET = 0 / ENABLEOFFSET between OBJECT frames WARP_WX =170 / DISTANT BETWEEN NODES ALONG X WARP_WY = 30 / DISTANT BETWEEN NODES ALONG Y WARP_DEG= 3 / DEGREE FOR LINE CURVATURE CORRECTION FLAT_DX = 0 / SHIFT BETWEEN OBJ AND FLAT ALONG X FLAT_DY = 0 / SHIFT BETWEEN OBJ AND FLAT ALONG X FLAT_BLU= 00. / RED BORDER FOR FLAT NORMALIZATION CUT_DEG = 3 / DEGREE FOR TRAECTORY CUT_TOP = 399 / NUMBERS OF UPPER STROBS CUT_DOWN= 400 / NUMBERS OF DOWN STROBS CUT_WIN = '350,800' CUT_STEP= 1 / NUMBERS OF PX IN STROB OUT_WAVE= '' / LAMBDA_0,D_LAMBDA,N OUTPUT DATA N_DEG =4 / DEGREE OF THE DISPERSION CURVE FITTING Y_FIT = 0 / DEGREE OF THE FITTING ALONG SLIT LINEFWHM= 6 / FWHM OF THE NEON LINES SKY_REG ='0,185,615,799' / REGION FOR SKY (Y1,Y2,Y3,Y4) SKY_DEG = 4 / DEGREE OF SKY SUBTRACTION SKY_STAR='0,250,625,800' / REGION FOR SKY (Y1,Y2,Y3,Y4) for STAR TABLE = 'C:\Program Files\RSI\libMOIS\astro_libs\LONG\okestan\mbd25.dat' / FILENAME MAG TABLE STANDARD STAR YPOS_OBJ= '250,190,310' /YPOSITION OF OBJECT FOR EXTRACTION OBJFIRST= 560 /YPOSITION OF FIRST EXTRACTED OBJECT ON MAP EXTR_WIN= 5 /HALF OF WINDOW FOR EXTRACTION FILESLIT='' / SLIT POSITION END