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