Dear Frank,You are worthy of the honor
And thanks for IRAF group to help us using the powerful software to process the astronomical images very much.Following are the output for your reference:
[code:1:24fd5da8c5]ccdred> lpar ccdred ccdproc darkcombine [/code:1:24fd5da8c5]
ccdred:
(pixeltype = "real real") Output and calculation pixel datatypes
(verbose = yes) Print log information to the standard output?
(logfile = "logfile") Text log file
(plotfile = "") Log metacode plot file
(backup = "") Backup directory or prefix
(instrument = "") CCD instrument file
(ssfile = "subsets") Subset translation file
(graphics = "stdgraph") Interactive graphics output device
(cursor = "") Graphics cursor input
(version = "2: October 1987")
(mode = "ql")
($nargs = 0)
ccdproc:
images = "@f.list" List of CCD images to correct
(output = "") List of output CCD images
(ccdtype = "flat") CCD image type to correct
(max_cache = 0) Maximum image caching memory (in Mbytes)
(noproc = no) List processing steps only?\n
(fixpix = no) Fix bad CCD lines and columns?
(overscan = no) Apply overscan strip correction?
(trim = no) Trim the image?
(zerocor = yes) Apply zero level correction?
(darkcor = yes) Apply dark count correction?
(flatcor = no) Apply flat field correction?
(illumcor = no) Apply illumination correction?
(fringecor = no) Apply fringe correction?
(readcor = no) Convert zero level image to readout correction?
(scancor = no) Convert flat field image to scan correction?\n
(readaxis = "line") Read out axis (column|line)
(fixfile = "") File describing the bad lines and columns
(biassec = "image") Overscan strip image section
(trimsec = "image") Trim data section
(zero = "../bias/zero.fits") Zero level calibration image
(dark = "../dark/dark.fits") Dark count calibration image
(flat = "") Flat field images
(illum = "") Illumination correction images
(fringe = "") Fringe correction images
(minreplace = 1.) Minimum flat field value
(scantype = "shortscan") Scan type (shortscan|longscan)
(nscan = 1) Number of short scan lines\n
(interactive = yes) Fit overscan interactively?
(function = "chebyshev") Fitting function
(order = 1) Number of polynomial terms or spline pieces
(sample = "*") Sample points to fit
(naverage = 1) Number of sample points to combine
(niterate = 1) Number of rejection iterations
(low_reject = 3.) Low sigma rejection factor
(high_reject = 3.) High sigma rejection factor
(grow = 0.) Rejection growing radius
(mode = "ql")
darkcombine:
input = "@d.list" List of dark images to combine
(output = "dark") Output dark image root name
(combine = "average") Type of combine operation
(reject = "minmax") Type of rejection
(ccdtype = "dark") CCD image type to combine
(process = no) Process images before combining?
(delete = no) Delete input images after combining?
(clobber = no) Clobber existing output image?
(scale = "exposure") Image scaling
(statsec = "") Image section for computing statistics
(nlow = 0) minmax: Number of low pixels to reject
(nhigh = 1) minmax: Number of high pixels to reject
(nkeep = 1) Minimum to keep (pos) or maximum to reject (neg
(mclip = yes) Use median in sigma clipping algorithms?
(lsigma = 3.) Lower sigma clipping factor
(hsigma = 3.) Upper sigma clipping factor
(rdnoise = "8") ccdclip: CCD readout noise (electrons)
(gain = "1.4") ccdclip: CCD gain (electrons/DN)
(snoise = "0.") ccdclip: Sensitivity noise (fraction)
(pclip = -0.5) pclip: Percentile clipping parameter
(blank = 0.) Value if there are no pixels
(mode = "ql") [code:1:24fd5da8c5]ccdred> imhead Imager37.FIT,../bias/zero.fits |+ [/code:1:24fd5da8c5]
Imager37.FIT[2184,1472][ushort]:
No bad pixels, min=0., max=0. (old)
Line storage mode, physdim [2184,1472], length of user area 1215 s.u.
Created Thu 11:41:29 01-Nov-2007, Last modified Thu 11:41:33 01-Nov-2007
Pixel file "Imager37.FIT" [ok]
EXTEND = F / File may contain extensions
BSCALE = 1.000000E0 / REAL = TAPE*BSCALE + BZERO
BZERO = 3.276800E4 /
DATE = '2007-11-01T03:41:29' / Date FITS file was generated
IRAF-TLM= '11:41:33 (01/11/2007)' / Time of last modification
BIAS = 100
ORIGIN = 'Origin '
TELESCOP= '400mm 100mm '
FOCALLEN= +4.000000000000e+002
APERTURE= +1.000000000000e+002
OBSERVER= 'Lelis1 '
DATE-OBS= '2007-03-02 '
TIME-OBS= '10:23:35 '
CCDSFPT = 4
CCDSUBFL= 0
CCDSUBFT= 0
CCDXBIN = 1
CCDYBIN = 1
EXPSTATE= 293
TEMPERAT= -1.186874500521e+001
INSTRUME= 'SBIG ST-10/10XE '
E-GAIN = +1.390000000000e+000
XPIXSZ = +6.800000000000e-003
YPIXSZ = +6.800000000000e-003
SBIGIMG = 8
EXPOSURE= +1.500000000000e+001
CBLACK = 13942
CWHITE = 15649
IMAGETYP= 'flat '../bias/zero.fits[2184,1472][real]:
No bad pixels, min=0., max=0. (old)
Line storage mode, physdim [2184,1472], length of user area 1215 s.u.
Created Wed 11:58:54 31-Oct-2007, Last modified Wed 11:58:50 31-Oct-2007
Pixel file "../bias/zero.fits" [ok]
EXTEND = F / File may contain extensions
ORIGIN = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator
DATE = '2007-10-31T03:58:54' / Date FITS file was generated
IRAF-TLM= '11:58:50 (31/10/2007)' / Time of last modification
BIAS = 100
TELESCOP= '400mm 100mm '
FOCALLEN= +4.000000000000e+002
APERTURE= +1.000000000000e+002
OBSERVER= 'Lelis1 '
DATE-OBS= '2007-02-05 '
TIME-OBS= '23:05:06 '
CCDSFPT = 2
CCDSUBFL= 0
CCDSUBFT= 0
CCDXBIN = 1
CCDYBIN = 1
EXPSTATE= 293
TEMPERAT= -9.787817267812e+000
INSTRUME= 'SBIG ST-10/10XE '
E-GAIN = +1.390000000000e+000
XPIXSZ = +6.800000000000e-003
YPIXSZ = +6.800000000000e-003
SBIGIMG = 8
EXPOSURE= +0.000000000000e+000
CBLACK = 90
CWHITE = 154
IMAGETYP= 'zero '
NCOMBINE= 10
EXPTIME = 0.
DARKTIME= 0.
Thansk!!
hymong