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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3.3. NON-GRB PRODUCTS 17<br />
Figure 3.3 shows an example 1 second <strong>BAT</strong> rate light curve, with a typical background level and<br />
variation for a portion of the orbit. Swift spacecraft orbits which pass near the SAA can produce<br />
<strong>BAT</strong> rates as high as 10 5 counts per second.<br />
Mask tagged data are generated on-board by the <strong>BAT</strong> flight software, and contain a crude light<br />
curve of up to three astrophysical sources. <strong>The</strong>se sources are chosen automatically by the flight<br />
software at the time of data collection. <strong>The</strong> raw mask tagged data may be converted to background<br />
subtracted light curves using the batmasktaglc software task.<br />
3.3.3 Maps<br />
<strong>The</strong> <strong>BAT</strong> flight software periodically produces housekeeping maps which are useful for <strong>BAT</strong> analysis.<br />
<strong>The</strong> most important of these are detector enable/disable maps and gain/offset maps. Detector<br />
enable/disable maps represent which detectors have been automatically disabled. Usually detectors<br />
are disabled because they are noisy. <strong>The</strong> number of enabled detectors must be taken into<br />
account when performing mask weighting and image analysis.<br />
Gain/offset maps are produced by the automatic calibration system. <strong>The</strong>y record the approximate<br />
pulse-height-to-energy calibration for each detector. This map, in combination with ground<br />
calibration files, is used to produce calibrated event lists (using bateconvert) and survey files (using<br />
baterebin).<br />
Mask weight maps are associated with mask tagged rates, and are needed to produce background<br />
subtracted light curves. In the standard FITS products, mask weight maps should be<br />
attached to the mask tagged light curve files.<br />
3.3.4 Trend Products<br />
Various other tables and maps are generated as well. <strong>The</strong>se can be broken down into several broad<br />
categories:<br />
• detector maps used in on-board imaging (“scaled” maps);<br />
• calibration pulser maps used to produce gain/offset maps on-board;<br />
• trigger diagnostic tables for rate (long and short) and image trigger systems;<br />
• the on-board source catalog;<br />
• americium tagged-source spectra (“block spectra”) and survey-type data (“Americium DPHs”),<br />
which are used to calibrate the absolute energy scale;<br />
• science housekeeping (“DAP HK”), plus various diagnostics;<br />
• engineering housekeeping;<br />
• debug stream (an ASCII log of the flight software activities);<br />
As noted above, a more detailed description of the format and content of all the products can<br />
be found in Appendix A.