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
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<strong>6.3</strong>. OLD ISSUES 67<br />
1. Sources will appear to be at the wrong locations;<br />
2. Mask weighted fluxes for known sources will be lower, or zero,<br />
• since the known celestial position will translate to the incorrect detector position. This<br />
causes the mask weighting function to sample the PSF off-center, and thus reduces the<br />
response.<br />
Users with pre-launch files should download a revised set of CALDB files. (20041120 version 1<br />
or later).<br />
<strong>6.3</strong>.13 batbinevt: Incorrect EXPOSURE Keyword<br />
Task: batbinevt<br />
<strong>Version</strong>: 1.7 and earlier<br />
What Builds: Swift 1.1 and earlier (Build 11 and earlier)<br />
Problem: Incorrect EXPOSURE keyword written to spectral files<br />
Status: Closed (Swift 1.2)<br />
<strong>The</strong> batbinevt task makes spectra. It writes “Type II” files which can have multiple spectra<br />
per file. It writes an EXPOSURE column to record the exposure for each spectrum.<br />
However, the input event or survey file also has an EXPOSURE keyword, which was not being<br />
overwritten. Thus it was possible to have conflicting exposure values. Unfortunately, XPSEC uses<br />
the keyword (incorrect) value instead of the column (correct) value.<br />
This bug is fixed in Swift 1.2.<br />
Workaround. Remove the EXPOSURE keyword from the spectral file. Since the EXPOSURE<br />
column is still present, XSPEC will still work, and should report the correct fluxes and fluences.<br />
Commands to remove the EXPOSURE keyword from myfile.pha:<br />
fthedit myfile.pha EXPOSURE delete<br />
<strong>6.3</strong>.14 batcelldetect: Incorrect Error Bars<br />
Task: batcelldetect<br />
<strong>Version</strong>: 1.09 and earlier<br />
What Builds: Swift 1.1 and earlier<br />
Problem: Error bars reported by batcelldetect are too small by a factor of ∼4<br />
Status: Corrected for Swift 1.2<br />
Discussion: batcelldetect performs a PSF fit to detected sources in an input image. This fit is<br />
done with a least-squares routine. Errors are estimated by using the formal statistical error (i.e.<br />
covariance matrix). <strong>The</strong> problem is that the error bars were too small by a factor of ∼4 compared<br />
to the “true” values based on population analysis. This turned out to be because the images were<br />
oversampled by a factor of 2 in each dimension, which affects the statistics. batcelldetect attempted<br />
to account for the oversampling, but did it incorrectly in versions 1.09 and earlier.