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Abteilung Astronomie

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T_GROUP Source code in t_group.pro

T_GROUP

Name
       T_GROUP
Purpose
       Driver procedure (for GROUP) to place stars in non-overlapping groups.
Explanation
       This procedure is part of the DAOPHOT sequence that places star
       positions with non-overlapping PSFs into distinct groups
       Input and output are to FITS ASCII tables
Calling Sequence
       T_GROUP, fitsfile, [ rmax, XPAR = , YPAR = , NEWTABLE = ]
Input Parameters
       FITSFILE -  Name of disk FITS ASCII table containing the X,Y positions
               in FITS (FORTRAN) convention (first pixel is 1,1)
Optional Input Parameters
       rmax - maximum allowable distance between stars in a single group
Optional Input Keywords
       XPAR, YPAR - scalar strings giving the field name in the output table
               containing the X and Y coordinates.   If not supplied,
               then the fields 'X' and 'Y' are read.
       NEWTABLE - scalar giving name of output disk FITS ASCII table.   If not
               supplied,
Procedures Used
       FTADDCOL, FTGET(), FTINFO, FTPUT, GROUP, READFITS(), SXADDHIST,
       SXADDHIST, WRITEFITS
Revision History
       Written, W. Landsman        STX Co.      May, 1996
       Converted to IDL V5.0   W. Landsman   September 1997
       Updated for new FTINFO call    W. Landsman    May 2000

Last modified by pro2html on 2001 April 26 at 03:13 UTC

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Jörn Wilms (wilms@astro.uni-tuebingen.de)
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