-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[<brightmagnitude>]<faintmagnitude>
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 polynomial solution.