File: imusa2.1

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.TH imusa2 1 WCS "14 April 1998"
.SH Name
imusa2 \- Find USNO-SA2.0 stars in FITS or IRAF image files
.SH Synopsis
imua2 [options] FITS or IRAF file(s)
.SH 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.
.SH Options
.TP
.B \-b [<RA> <Dec>]
Output in B1950, optional new image center in B1950 (FK4) RA and Dec
.TP
.B \-h
Print heading, else do not 
.TP
.B \-j [<RA> <Dec>]
Output in J2000, optional new image center in J2000 (FK5) RA and Dec
.TP
.B \-m [<bright magnitude>] <faint magnitude>
Limiting catalog magnitude(s) (default none, bright \-2 if only faint is given)
.TP
.B \-n <num>
Number of brightest stars to print 
.TP
.B \-p <scale>
Initial plate scale in arcsec per pixel (default 0)
.TP
.B \-s
Sort by RA instead of flux 
.TP
.B \-t
Tab table to standard output as well as file
.TP
.B \-u
USNO catalog single plate number to accept
.TP
.B \-v
Verbose listing of processing intermediate results
.TP
.B \-w
Write tab table output file imagename.cat
.B \-z
Use AIPS classic projections instead of WCSLIB; use CD matrix or CDELT
instead of polynomial solution.
.SH See Also
imcat(),imgsc(),imua2(),scat()
.SH Web Page
http://tdc-www.harvard.edu/software/wcstools/imcat/imusa2.html
.SH Author
Jessica Mink, SAO (jmink@cfa.harvard.edu)