SIMPLE  =   T / LONG-SLIT DATA REDUCTION
R_DIR   =  '~/obs/scorpio/s111120/'      / DIRECTORY FOR READING DATA
W_DIR   =  '~/obs/processed/scorpio/sunsky_111120/' / DIRECTORY FOR WRITING DATA
NIGHT   =  s937                / NUMBER OBSERVING NIGHT
CCD_CUT = '500,1,4625,1020'   / REGION WITHOUT OVERSCAN (X0,Y0,X1,Y1)
CUB_OBJ = '01'                         
CUB_STAR= ''
CUB_NEON= '01'
CUB_FLAT= '01'
OBJ     = '01,02,03'  / NUMBERS OBJECT FILES
NEON    = '04'           / NUMBERS COMPARISON SPECTRUM FILES
FLAT    = '05,06'           / NUMBERS FLAT FILES
FL_MASK = '07'
MAP     = ''
\\\\\\\\\\\\\ Y SOLUTION CONSTRUCTION ///////////////
NDOTS   = 13
XDEG    = 4
YDEG_Y  = 2
\\\\\\\\\\ WAVE SOLUTION CONSTRUCTION //////////////
FLINES  = '~/sci/IDL_libs/HeNeAr_spec/linesHeNeAr_SCORPIO_chil_autopipline.tab' 
LWIN    = '4044.42, 4471.81,5015.68, 5852.5, 6143.1, 6402.25, 7245.17' /strongest emission lines in yline 600 for neon file
PX      = ' 210    ,  796   ,1476,    2452,   2784  , 3079   , 4045' /their px coordinates
SPRAN   = '3900,7300' /spectral range
WIN0    = 20.0  /width in px for preliminary line searching
NYREG   = 30 /number of region in Y direction
DEG0    = 3 /degree of polinomials described preliminary dispersion curve
DEG1    = 5 /degree of dispersion curve
YDEG_W  = 2 /degree of  in Y-direstion
MINNLINE= 40 / minimum number if lines for detection
MAXERR  = 0.12 / maximumal acceptable error in line
\\\\\\\\\\\ NIGHT SKY /////////////////
LSFDIR  = '/media/06A0AA5BA0AA514B/obs/work/for_Zasov/n524/ScRed_sunsky_pa217/'
SKYPOS  = '55,130,200,300,800,880, 915, 1023' /
POSWID  = '15'
FILFACT = 5
BKSPC   = 1.0  /parameter of B-spline solution, distance between knots in A
DEGMOD  = 550  / number basis functions
SIGREC  = 0
\\\\\\\\ CORRECT DISPERSION DIRECTION //////////////
DEGPO   = 2
END