You are here: Home / Surveys & Projects / Software Release / WCS fitting

WCS fitting

wcsfit matches up objects from an image with astrometric position standards. The transformation between the cartesian and equatorial coordinates is fit. The results are written in both the image header and the catalogue table header in the standard FITS header keywords. A FITS image and an imcore generated catalogue are required input. By default the objects in the catalogue are matched to 2MASS standards which is extracted from the CASU mirror of VizieR. This can be changed by using the optional switches described below.

If the input image is a multiextension FITS file, then the number of extensions in the input catalogue must match with the number of image extensions. wcsfit will fit each image extension in turn.

SYNOPSIS

wcsfit infile incat

ARGUMENTS

infile 
Input FITS image. 
incat 
Input FITS table which has been generated by imcorewith source extraacted from infile

OPTIONS

The following options are supported.  Default values are specified after th e equal sign.

--catsrc=viz2mass
This is the source of the standard stars to be used in the astrometric fit. The following values are supported:
viz2mass
2MASS standards are extracted from a VizieR distribution defined by --site.
vizusnob
USNOB standards are extracted from a VizieR distribution defined by --site.
vizlandolt
Landolt standards are extracted from a VizieR distribution defined by .
local2mass
A local FITS copy of the 2MASS catalogue is searched. The full path to the FITS files is defined by --catpath
localusnob
A local copy of the USNOB catalogue is searched. The full path to the .cat and .acc files is defined by --catpath.
localfits
A locally available FITS table will be searched. The full path to this table is given by --catpath. The only which are required in the table are ra and dec. Both of these must be in degrees.
--site
In the event that a VizieR distribution is being used by --catsrc, then this defines the site of the distribution. Currently two values are supported: casu uses the VizieR mirror at CASU in Cambridge and CDS uses the original VizieR at CDS.
--catpath
In the event that a local option is specified in the value for --catsrc this defines the full path to the file(s).