Linux and UNIX Man Pages

Linux & Unix Commands - Search Man Pages

scat(1) [debian man page]

scat(1) 						      General Commands Manual							   scat(1)

Name
       scat - Find catalog stars in a square or circle on the sky

Synopsis
       scat [options] [-b or -j] ra dec

Description
       scat  is  a  utility for finding all of the Hubble Space Telescope Guide Star Catalog (GSC), U.S. Naval Observatory A2.0 (UA2), B1.0 (UB1),
       SA2.0 (USA2), or UJ (UJC) Catalogs, or locally catalogued objects in a specified region of the sky and listing  their  sky  coordinates	to
       standard  output. If the -w flag is set, they are written to a file objectname.catalogname, where objectname is given by the argument to -o
       on the command line, defaulting to "search", and catalogname is given by the argument to -c on the command line. The  catalog  defaults	to
       the  GSC,  if no -c argument is present. scat resembles rgsc(1) and star(1), which can search from lists of coordinates but cannot sort the
       output.	sgsc, suac, and susac are links to this program.1

Options
       -a     List the single closest catalog source

       -b <RA> <Dec>
	      Output B1950 (FK4) coordinates around this center

       -c <name>
	      Reference catalog (gsc(=HST GSC), ua2(=USNO-A2.0), TMC(=2MASS Point Source Catalog), gsc2(=GSC  II),  ub1(=USNO-B1.0),  local  file,
	      etc.)

       -d
	       Output RA and Dec in degrees instead of hh:mm:ss dd:mm:ss

       -e     Output ecliptic coordinates

       -f     Output search center for other programs

       -g <class>
	      HST Guide Star Catalog object class (0=stars 3=galaxies -1=all)

       -h     Print search and column heading, else do not

       -i     Print catalog object name, not catalog number

       -j <RA> <Dec>
	      Output J2000 (FK5) coordinates around this center

       -k <keyword>
	      Add value of this keyword to end of output lines from a tab table search

       -l     Print search center and closest star on one line

       -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

       -o <name>
	      Object name used for output file naming

       -q <year>
	      Equinox of output position in fractional years

       -r <radius>
	      Halfwidth (-radius if negative) of search area in arcseconds (default 10)

       -s d|m|n|p|r
	      Sort by (d)eclination, (m)agnitude, (n)o sort, (p)distance from center, or (r)ight ascension.

       -t     Tab table to standard output or file

       -u <x> <y>
	      Print x y instead of number in front of non-tab output, before RA and Dec or add x and y columns to end of tab output line

       -v     Verbose listing of processing intermediate results

       -w     Write output file objectname.catalog or search.catalog if -o is not used.

       -x <type>
	      GSC object type (0=stars 3=galaxies -1=all -2=bands)

       -y <year>
	      Epoch of output positions in fractional years (for proper motion only)

       -z     Append to existing output file search.catalog or objectname.catalog.  Start file if it does not already exist.

See Also
       imcat()

Web Page
       http://tdc-www.harvard.edu/software/wcstools/scat/

Author
       Doug Mink, SAO (dmink@cfa.harvard.edu)

30 January 2003 						     WCSTools								   scat(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)
Man Page