imusa2(1) [debian man page]
imusa2(1) General Commands Manual imusa2(1) Name imusa2 - Find USNO-SA2.0 stars in FITS or IRAF image files Synopsis imua2 [options] FITS or IRAF file(s) Description Search USNO-SA2.0 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 imcat(),imgsc(),imua2(),scat() Web Page http://tdc-www.harvard.edu/software/wcstools/imcat/imusa2.html Author Doug Mink, SAO (dmink@cfa.harvard.edu) 14 April 1998 WCS imusa2(1)
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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)