SIMPLE = T / LONG-SLIT DATA REDUCTION R_DIR = 'g:\obs_data\s090404\' / DIRECTORY FOR READING DATA W_DIR = 'H:\long\NGC2950\VPGH1800R\N2950_PA29' / DIRECTORY FOR WRITING DATA NIGHT = S654 / NUMBER OBSERVING NIETH CCD_CUT = '20,0,2067,1023' / REGION WITHOUT OVERSCAN (X0,Y0,X1,Y1) CUB_OBJ = '04' CUB_NEON= '04' CUB_FLAT= '04' CUB_STAR= '04' OBJ = '03,04,05' / NUMBERS OBJECT FILES FLAT = '07,08' / NUMBERS FLAT FILES NEON = '02,06' / NUMBERS COMPARISON SPECTRUM FILES STAR = '04' /NUMBERS STAR FILES OBJ_XSHI= 1 / ALLOW SHIFT along X OFFSET = 0 /OFFSET between OBJECT frames WARP_WX =210 / DISTANT BETWEEN NODES ALONG X WARP_WY = 30 / DISTANT BETWEEN NODES ALONG Y WARP_DEG= 2 / 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 = 2 / DEGREE FOR TRAECTORY CUT_TOP = 400 / NUMBERS OF UPPER STROBS CUT_DOWN= 400 / NUMBERS OF DOWN STROBS CUT_WIN ='' CUT_STEP= 1 / NUMBERS OF PX IN STROB OUT_WAVE= '6120,0.5,2000' / LAMBDA_0,D_LAMBDA,N OUTPUT DATA N_DEG = 3 / DEGREE OF THE DISPERSION CURVE FITTING Y_FIT = 0 / DEGREE OF THE FITTING ALONG SLIT LINEFWHM= 5 / FWHM OF THE NEON LINES SKY_REG ='0,320,480,800' / REGION FOR SKY (Y1,Y2,Y3,Y4) SKY_DEG = 2 / DEGREE OF SKY SUBTRACTION SKY_STAR='250,380,490,550' / REGION FOR SKY (Y1,Y2,Y3,Y4) for STAR USE5577 = 0 /USING SKY LINE 5577 FOR WAVELENGTH CALIBRATION TABLE = 'c:\okestan\mfeige56.dat' / FILENAME MAG TABLE STANDARD STAR YPOS_OBJ= '400' /YPOSITION OF OBJECT FOR EXTRACTION OBJFIRST= '544' /YPOSITION OF FIRST EXTRACTED OBJECT ON MAP EXTR_WIN= 10 /HALF OF WINDOW FOR EXTRACTION END