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cphead(1) [debian man page]

CPHEAD(1)							   User Commands							 CPHEAD(1)

NAME
cphead - AME SYNOPSIS
cphead [-v][-d dir][-p num] file1.fit ... filen.fits kw1 kw2 ... kwn DESCRIPTION
Copy FITS or IRAF header keyword values from first file to others or : cphead [-v][-d dir][-p num] file1.fit @filelist kw1 kw2 ... kwn or : cphead [-v][-d dir][-p num] file1.fit @filelist @kwlist -a: Replace header of 2nd file with that from first -d: Root directory for input files (default is cwd) -h: Write HISTORY line -k: Write CPHEAD keyword -n: Write a new file (add e before the extension) -p: Number of decimal places in numeric output -v: Verbose -w: Copy all WCS keywords cphead 3.8.4 June 2012 CPHEAD(1)

Check Out this Related Man Page

WCSREMAP(1)							   User Commands						       WCSREMAP(1)

NAME
wcsremap - AME SYNOPSIS
remap [-vf][-a rot][[-b][-j] ra dec][-i bits][-l num] file1.fit file2.fit ... filen.fit DESCRIPTION
Remap FITS or IRAF images into single FITS image using WCS or : remap [-vf][-a rot][[-b][-j] ra dec][-i bits][-l num] @filelist -a: Output rotation angle in degrees (default 0) -b ra dec: Output center in B1950 (FK4) RA and Dec -e long lat: Output center in ecliptic longitude and latitude -f file: Use WCS from this file as output WCS -g long lat: Output center in galactic longitude and latitude -i num: Number of bits per output pixel (default is input) -j ra dec: center in J2000 (FK5) RA and Dec -l num: Log every num rows of output image -m mode: c closest pixel (more to come) -n num: integer pixel value for blank pixel -o name: Name for output image -p secpix: Output plate scale in arcsec/pixel (default =input) -s: Set BZERO and BSCALE in output file from input file -t: Number of samples per linear output pixel -u: Delete distortion keywords from output file -v: Verbose -w type: Output WCS type (input is default) -x x y: Output image reference X and Y coordinates (default is center) -y nx ny: Output image dimensions (default is first input image) wcsremap 3.8.4 June 2012 WCSREMAP(1)
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