NAME

USAGE

DESCRIPTION

The primary output HDU contains keywords taken from the primary input HDU. The first extension of the output contains the summed image.

PARAMETERS

infile [filename]

FITS input UVOT image file. This can be a raw (sw*u??_rw.img) or sky (sw*u??_sk.img) image file. Appropriate keywords from the input HDUs are propagated to the output. If the input is an aspect corrected sky image file, the output will have the same corrections applied.

outfile [filename]

Name of output file. If not NONE, this will hold sky LSS maps.

(attfile = NONE) [filename]

Name of attitude file.

(teldeffile = CALDB) [filename]

Name of TELDEF file or CALDB.

(alignfile = CALDB) [filename]

Name of ALIGN file or CALDB.

(lssfile = CALDB) [filename]

Name of SKYFLAT file or CALDB.

(rawfile = NONE) [filename]

Name of output raw LSS maps or NONE.

(sumfile = NONE) [filename]

Name of output raw LSS maps or NONE.

(exclude = DEFAULT) [string]

This parameter is passed through to uvotimsum.

(maskfile = NONE) [string]

This parameter is passed through to uvotimsum.

(cleanup = yes) [boolean]

Remove temporary files?

(clobber = no) [boolean]

Overwrite existing output file?

(history = yes) [boolean]

Write parameters to history keywords?

(chatter = 3) [enumerated integer]

Standard HEAdas chatter parameter.

EXAMPLES

1. Run uvotskylss specifying the input sky image file and output sky LSS file. The output file will have parallel structure to the input file and keywords in the output SKY HDUs will match those in the input HDUs

      uvotskylss infile=swuv_sk.img outfile=swuv_sklss.img

      uvotskylss infile=swuv_sk.img outfile=NONE sumfile=swuv_sklsssum.img

SEE ALSO

LAST MODIFIED