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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5.8. MAKING <strong>BAT</strong> SKY IMAGES 49<br />
5.8.5 Making a Background Detector Plane Image<br />
Making a background detector plane image is optional, but it will increase the sensitivity of the<br />
image when bright sources are present. If possible, the background interval should be made from<br />
data with similar background levels and for a longer duration than the source image.<br />
Use the same procedure as above to create a DPI file during a time range when you know there<br />
is no source emission. Let us call that file “bkg.dpi”.<br />
NOTE: if the background or bright sources are known to have varied significantly between the<br />
time of the source and background DPIs, there may be little or no benefit to making a background<br />
file.<br />
Advanced usage: if bright sources are known to be present in the image, it is possible to use<br />
the batclean task to create a background map which removes many systematic artifacts. This is<br />
usually not necessary for images with exposures less than 100 seconds.<br />
5.8.6 Making a Sky Image<br />
A sky image is created from a DPI using the ‘batfftimage’ task. Issue the following command,<br />
batfftimage infile=flare.dpi outfile=flare.img attitude=../../auxil/sw00145675000sat.fits.gz \<br />
bkgfile=bkg.dpi detmask=../hk/sw00145675000bcbdq.hk.gz clobber=YES<br />
where<br />
• infile is the DPI file name<br />
• bkgfile is the background DPI file name (‘NONE’ can also be used if no background file is<br />
available)<br />
• outfile is the output sky image file name<br />
• attitude is the spacecraft attitude file name<br />
• detmask is the detector quality map<br />
<strong>The</strong> result is a <strong>BAT</strong> sky image. If valid spacecraft attitude data was used, then the sky image<br />
should automatically have celestial coordinates (WCS keywords) attached.<br />
You may use your favorite FITS image viewer to examine the image (for example FV or DS9).<br />
Figure 5.6 shows the appearance of a typical bright point source in a <strong>BAT</strong> sky image.<br />
5.8.7 Caveats<br />
<strong>The</strong> spacecraft attitude may have changed during the accumulation interval of your DPI. You must<br />
carefully filter out spacecraft slew data and use only steady pointed attitude information, or the<br />
celestial coordinate system will be erroneous.