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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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16 CHAPTER 3. <strong>BAT</strong> OPERATING MODES AND DATA TYPES<br />

Figure 3.3: Example of <strong>BAT</strong> 1 second rates. All variations shown are due to the space environment<br />

and not an astrophysical source.<br />

<strong>The</strong> rate data include:<br />

• one-second rates (1 sec sampling; full energy band; full array);<br />

• 64 msec rates (64 msec sampling; four energy bands; full array);<br />

• quadrant rates (1.6 sec sampling; four energy bands; four separate spatial quadrants);<br />

• mask-tagged rates (1.6 sec sampling; four energy bands; three distinct sources);<br />

• maximum rates (maximum counts recorded for multiple time scales, energy bands and<br />

spatial regions).<br />

All rate data except for mask-tagged rate data are not background subtracted. This means<br />

that the hard X-ray background and particle backgrounds are included in the rates. Also, since<br />

there is no per-detector information recorded in the rate data, it is possible for noisy detectors to<br />

generate rapid spikes which may emulate a gamma-ray burst or other rapidly varying phenomenon.<br />

Thus, while rate variations may be suggestive of an astrophysical event, conclusive proof must be<br />

obtained from image analysis.

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