NAME:
tmplinfo
PURPOSE: (one line only)
Generate information about a template image based on an image header
DESCRIPTION:
CATEGORY:
CCD data processing
CALLING SEQUENCE:
tmplfn,input,info
INPUTS:
input - There are two options for input.
1 - a scalar string that is the name of the image file. This
should include the path if the file cannot be found in
the current directory.
2 - a string array with the FITS header from an image file.
OPTIONAL INPUT PARAMETERS:
KEYWORD INPUT PARAMETERS:
KEYLIST - Name of a file containing a correspondence list. This list
associates a set of standard names with the actual keyword
names found in a FITS file header. If this keyword is
omitted, a default list is used, as if a file with the
following contents had been supplied:
AIRMASS K AIRMASS
DATE K DATE-OBS
DATETMPL T DD-MM-YYYY
EXPDELTA V 0.0
EXPTIME K EXPTIME
FILTER K FILTERS
FILENAME K CCDFNAME
OBJECT K OBJECT
UT K UT
RA K RA
DEC K DEC
The middle column is a flag. It may be K, for Keyword,
T, for Template, or V, for Value. If it is V, the contents
of the third field on that line should make sense for the
name in the first field.
OUTPUTS:
info - Anonymous structure with information about a template image
if constructed from this data image. This information is
intended to help with populating the refim and template
database tables.
error - Flag, if set indicates there was an error building the desired
information structure. In this case the info structure
is ill defined. If error is not set then everything is fine.
KEYWORD OUTPUT PARAMETERS:
COMMON BLOCKS:
SIDE EFFECTS:
RESTRICTIONS:
The image header must contain the astrometric solution in a form
compatible with astinfo.pro
PROCEDURE:
MODIFICATION HISTORY:
2010/08/06, Written by Marc W. Buie, Southwest Research Institute