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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12 CHAPTER 3. <strong>BAT</strong> OPERATING MODES AND DATA TYPES<br />
Figure 3.1: <strong>BAT</strong> data products for a typical GRB with a slew.<br />
<strong>BAT</strong> Rate Trigger Fast-rising GRBs lead to a rate trigger. A TDRSS “Alert” message may be<br />
sent to the ground.<br />
<strong>BAT</strong> Image Confirmation <strong>The</strong> image processing step takes several seconds. If a significant<br />
new excess is detected, then a GRB is declared, and a TDRSS position message is sent to the<br />
ground.<br />
<strong>BAT</strong> Image-only Trigger <strong>The</strong> <strong>BAT</strong> regularly performs image analysis, on roughly 1 minute,<br />
5 minute, and snapshot-duration accumulations, looking for new sources regardless of the<br />
rate trigger status. If a new excess is detected, it may be declared a GRB or a “transient”<br />
depending on the duration.<br />
Spacecraft Slew <strong>The</strong> spacecraft may or may not slew, depending on the merit of the burst<br />
and the observing constraints. <strong>The</strong> <strong>BAT</strong> products should be the same regardless of whether<br />
or not there is a slew. However, there will only be XRT and UVOT data if the slew occurs.<br />
<strong>BAT</strong> TDRSS Light Curve <strong>The</strong> <strong>BAT</strong> produces a total rate quick-look light curve of several<br />
hundred seconds around the time of the trigger. This light curve is acceptable for looking for<br />
crude features, but cannot be trusted for sensitive analysis, since the rates are contaminated<br />
by background events. This is especially a problem during the slew, when sources pass into<br />
and out of the <strong>BAT</strong> field of view, which causes rate variations.<br />
<strong>BAT</strong> Event Data This is the most relevant and useful data for GRB analysis, since it allows<br />
background to be removed via “mask weighting.” Also, the user can choose any source<br />
position, temporal or spatial binning that they desire. GRB light curves and spectra can be<br />
extracted during the spacecraft slews as well as pointings. Note that the <strong>BAT</strong> event data<br />
may overlap in time with nearby survey intervals.<br />
<strong>The</strong> response process and products as a function of time during a GRB are illustrated in Figure<br />
3.1. Note that even if the spacecraft does not slew, or slews to another target (not the GRB