SIMPLE = T / LONG-SLIT DATA REDUCTION R_DIR = 'd:\obs\s091010\' / DIRECTORY FOR READING DATA W_DIR = 'D:\obs\work\for_Zasov\n524\pa240\' / DIRECTORY FOR WRITING DATA NIGHT = S698 / NUMBER OBSERVING NIGHT CCD_CUT = '22,1,2066,1024' / REGION WITHOUT OVERSCAN (X0,Y0,X1,Y1) CUB_OBJ = '03' CUB_STAR= '04' CUB_NEON= '03' CUB_FLAT= '03' OBJ = '08,09,10,11,13,14,15,16,18,19,20,21' / NUMBERS OBJECT FILES FLAT = '23,24' / NUMBERS FLAT FILES NEON = '12,17,22' / NUMBERS COMPARISON SPECTRUM FILES STAR = '03' / NUMBERS STAR FILES OBJ_XSHI= 0 / ENABLE SHIFT along X OFFSET = 0 / ENABLEOFFSET between OBJECT frames WARP_WX =180 / 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 =6 / DEGREE OF THE DISPERSION CURVE FITTING Y_FIT = 0 / DEGREE OF THE FITTING ALONG SLIT LINEFWHM= 4 / FWHM OF THE NEON LINES SKY_REG ='120,240,550,730' / REGION FOR SKY (Y1,Y2,Y3,Y4) SKY_DEG = 4 / DEGREE OF SKY SUBTRACTION SKY_STAR='0,150,650,799' / REGION FOR SKY (Y1,Y2,Y3,Y4) for STAR TABLE = 'c:\IDL_libs\libMOIS\astro_libs\LONG\okestan\mhz2.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