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)
Check Out this Related Man Page
imua2(1) General Commands Manual imua2(1)Name
imua2 - Find USNO-A2.0 stars in FITS or IRAF image files
Synopsis
imua2 [options] FITS or IRAF file(s)
Description
Search USNO-A2.0 Catalog within the area described by the world coordinate system in an image header. This is a link to imcat rather than
a separate executable.
Options-b [<RA> <Dec>]
Output in B1950, optional new image center in B1950 (FK4) RA and Dec
-h Print heading, else do not
-j [<RA> <Dec>]
Output in J2000, optional new image center in J2000 (FK5) RA and Dec
-m [<bright magnitude>] <faint magnitude>
Limiting catalog magnitude(s) (default none, bright -2 if only faint is given)
-n <num>
Number of brightest stars to print
-p <scale>
Initial plate scale in arcsec per pixel (default 0)
-s Sort by RA instead of flux
-t Tab table to standard output as well as file
-u USNO catalog single plate number to accept
-v Verbose listing of processing intermediate results
-w Write tab table output file imagename.cat -z Use AIPS classic projections instead of WCSLIB; use CD matrix or CDELT instead of poly-
nomial solution.
See Also
imgsc(),imuac(),imusac(),scat()
Author
Doug Mink, SAO (dmink@cfa.harvard.edu)
Options-b [<RA> <Dec>]
Output B1950 (FK4) coordinates (optional center)
-u <plate>
Accept only stars from this plate (default all)
-h Print heading, else do not
-j [<RA> <Dec>]
Output J2000 (FK5) coordinates (optional center)
-m [<bright magnitude>] <faint magnitude>
Limiting catalog magnitude(s) (default none, bright -2 if only faint is given)
-n <num>
Number of brightest stars to print
-p <scale>
Plate scale in arcsec per pixel (default 0)
-s Sort by RA instead of flux
-t Tab table to standard output as well as file
-u <plate>
Accept only stars from thsi plate (default all)
-v Verbose listing of processing intermediate results
-w Write tab table output file imagename.uac
See Also
imcat(),imgsc(),imusa2(),scat()
Web Page
http://tdc-www.harvard.edu/software/wcstools/imcat/imua2.html
Author
Doug Mink, SAO (dmink@cfa.harvard.edu)
14 April 1998 WCS imua2(1)