NAME

USAGE

DESCRIPTION

uvotgcn manages running Swift UVOT software to process UVOT TDRSS packets.

The input packets are FITS files and are accompanied by text pseudo-GCN notices which contain position and error information.

The possible output products are three FITS files: a sky image, a list of sources, and a list of sources correlated against a star catalog; and a Postscript finding chart (field). The catalog file is only created if the source positions are successfully matched to the catalog.

PARAMETERS

packetfile [filename]

Name of the FITS file containing the UVOT TDRSS packet.

batfile [filename]

Name of the input pseudo BAT position notice.

xrtfile [filename]

Name of the input pseudo XRT position notice.

blcfile [filename]

Name of the input pseudo BAT light curve position notice.

catspec [filename]

Name of the catalog desciptor.

(lockfile = uvotgcn.lock) [filename]

File used to synchronize access to the input files.

(skyfile = DEFAULT) [filename]

Name of the output FITS sky image.

(sourcesfile = DEFAULT) [filename]

Name of the output FITS source table.

(catalogfile = DEFAULT) [filename]

Name of the output FITS source table correlated using catspec.

(fieldfile = DEFAULT) [filename]

Name of the output annotated Postscript finding chart or NONE.

(signalfile = DEFAULT) [filename]

Name of the packet processing complete signal file.

(timeout = 20) [int]

Maximum time to wait for sky image before timing out [sec].

(starid = NONE) [string]

Parameters to pass to star identification.

(stale = 500) [int]

Maximum age of pseudo-notices to load [sec].

(archive = uvotdata) [directory]

Location of UVOT TDRSS processing archive.

(remote = no) [boolean]

Transfer job for remote processing?

(chatter = 1) [integer, 0 - 5]

Standard HEAdas verbosity parameter.

EXAMPLES

1. Execute uvotgcn providing a UVOT TDRSS packet

	uvotgcn packetfile=swmsufc.fits

SEE ALSO

LAST MODIFIED