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diff --git a/noao/digiphot/daophot/doc/pfmerge.hlp b/noao/digiphot/daophot/doc/pfmerge.hlp new file mode 100644 index 00000000..a85b60ee --- /dev/null +++ b/noao/digiphot/daophot/doc/pfmerge.hlp @@ -0,0 +1,65 @@ +.help pfmerge May00 noao.digiphot.daophot +.ih +NAME +pfmerge -- merge a list of photometry files +.ih +USAGE +pfmerge inphotfiles outphotfile +.ih +PARAMETERS +.ls inphotfiles +The list of photometry files to be merged. Inphotfiles may be the output of the +DAOPHOT tasks PHOT, PSTSELECT, PSF, PEAK, GROUP, GRPSELECT, NSTAR, or ALLSTAR. +Inphotfiles may be either a list of APPHOT/DAOPHOT text databases or a list of +STSDAS binary tables. +.le +.ls outphotfile +The output photometry file. Outphotfile consists of the header of the first +input photometry file, followed by a list of records, one per input file +record, each consisting of five fields: ID, XCENTER, YCENTER, MAG, and MSKY. +Outphotfile is a an APPHOT/DAOPHOT text database if the first photometry file +is a text database, an STSDAS binary table if the first photometry file is an +ST table. +.le +.ls verbose +Print messages about the progress of the task ? +.le +.ih +DESCRIPTION +PFMERGE creates a new photometry file suitable for input to PSF, PEAK, GROUP, +or ALLSTAR by extracting the header of the first input photometry file and the +values of the five fields: ID, XCENTER, YCENTER, MAG, and MSKY from each +photometry record in each input file, and writing them to \fIoutphotfile\fR. +\fIInphotfiles\fR may be either APPHOT/DAOPHOT text databases or STSDAS binary +tables, but \fIoutphotfile\fR inherits the type of the first input photometry +file. + +The principal application of PFMERGE is to combine the results of one of the +DAOPHOT fitting tasks, e.g. ALLSTAR, with the results of the aperture photometry +task PHOT, to create a new photometry file suitable for input to the fitting +task. e.g. ALLSTAR, since it if often the case that the user wishes to combine +preliminary results for a few additional stars with the best fit results to +date on the original star list. + +PFMERGE is intended to combine photometry files from different DAOPHOT tasks. +The task PCONCAT can be used to combine photometry files produced by the same +task. + +.ih +EXAMPLES + +1. Combine the results of the first allstar run with phot task results +on a small list of stars detected after the first list of stars was +subtracted from the original image. + +.nf + cl> pfmerge m92.als.1,m92.mag.5 m92.als.2 +.fi +.ih +TIME REQUIREMENTS +.ih +BUGS +.ih +SEE ALSO +pconcat +.endhelp |