The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
110 APPENDIX D. <strong>BAT</strong> SOFTWARE TOOL REFERENCE<br />
map need not be an actual partial coding map; any quantity that can be thresholded (even<br />
a map of 0s and 1s) can be used. If pcode file is “NONE”, then the entire image is searched.<br />
(pcodethresh=0.01) [real ]<br />
Partial coding threshold for source detection. This threshold is applied to the map specified<br />
in pcodefile. Any partial coding value greater than pcodethresh is considered active for the<br />
purposes of source detection.<br />
(bkgpcodethresh=-1) [real ]<br />
Partial coding threshold for background analysis. This threshold is applied to the map specified<br />
in pcodefile. Any partial coding value greater than bkgpcodethresh is considered active<br />
for the purposes of measuring the backgroud and its variance. A value of -1 indicates that<br />
bkgpcodethresh should be set to pcodethresh. <strong>The</strong> “source” and “background” thresholds<br />
are kept separately so that background analysis can be done over a wider area than the source<br />
acceptance region.<br />
(pospeaks=YES) [boolean ]<br />
Constrain newly detected peaks to be positve. If NO, then significant positive or negative<br />
deviations will be searched for. Known catalogged sources are permitted to have a negative<br />
fitted flux regardless of pospeaks.<br />
(vectorflux=NO) [boolean ]<br />
If YES, then output flux values for a given source as a vector, one element for each input<br />
image. If NO, then output one catalog rows for each source in each input image. Note, for<br />
vectorflux=YES, the input images must all match their coordinate systems, exposure, and<br />
instrument configuration exactly.<br />
(rows = “-”) [string ]<br />
An index list of images to operate on. This is a standard comma-separated list of image<br />
ranges, starting with image number 1. Image number 1 corresponds to the primary extension<br />
of the input FITS file, 2 to the next extension, and so on. A range of “-” indicates all<br />
images should be processed. Thus, this parameter really selectsimage extension numbers<br />
to operate on rather than binary table rows.<br />
(niter=2) [integer ]<br />
Number of iterations of source detection to perform. niter=0 is allowed; in that case the<br />
sources in the input catalog (if any) which are in the field of view are transferred to the<br />
output catalog.<br />
(carryover=YES) [boolean ]<br />
For the analysis of multiple images. If YES, then carry over the sources detected in the<br />
analysis of earlier images to the analysis of later images. Positions of previously detected<br />
new sources are held fixed as described above. If NO, then the analysis of each image begins<br />
from scratch, excluding any previously detected sources. Note that carryover=NO and<br />
vectorflux=YES are contradictory.<br />
(nadjpix=3) [integer ]<br />
Minimum number of adjacent pixels required for source detection. This serves to decrease the<br />
number of false detections. This quantity is somewhat dependent on the image oversampling<br />
used.