30.01.2013 Views

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

A.6. MAPS 75<br />

A.6.2 Detector Quality Map<br />

A detector quality map file (code “dqcb”) is a ground-derived product. <strong>The</strong> primary extension<br />

contains a quality map indicating which detectors should be used for science analysis and which<br />

should not (0=use; 1=discard). This file is typically the output of the bathotpix task, which<br />

combines the detector enable/disable map (see “Enable/Disable Map” above) and counts map<br />

which has been screened for noisy detectors.<br />

Layout. Detector quality file<br />

Extension Description<br />

Primary 286&times;173 Map; Detector quality map (0=good; 1=bad)<br />

BADPIX List of bad pixels<br />

Layout. List of bad pixels. EXTNAME = ‘BADPIX’<br />

Name Format [Units](Range) Comment<br />

TIME 1D [s] Start time of hot pixel counts map<br />

EXPOSURE 1D [s] Exposure of hot pixel counts map<br />

DET ID 1J (0:32767) Detector identification number<br />

DETX 1I [pixel](0:285) <strong>BAT</strong> X detector pixel number<br />

DETY 1I [pixel](0:172) <strong>BAT</strong> Y detector pixel number<br />

QUALITY 1I Detector quality flag<br />

COUNTS 1J [count] Number of counts in flagged detector<br />

<strong>The</strong> QUALITY flag can take the following values.<br />

QUALITY Meaning<br />

0 Good<br />

1 disabled detector<br />

2 cold or undersensitive detector<br />

3 hot or noisy detector<br />

A.<strong>6.3</strong> Gain / Offset Map<br />

Gain/offset maps (code “gocb”) are produced by the <strong>BAT</strong> on-board automatic calibration system,<br />

and provide the linear transformation from pulse height to keV. This map is used with other<br />

calibration files to produced calibrated energy values for event and survey data. While other nonlinear<br />

corrections should be applied, the basic calculation for a given detector is, PI [keV] = PHA<br />

[chan] * GAIN + OFFSET.<br />

Gain/offset maps are not always produced during every observation, but the Swift Data Center<br />

should collect the nearest map for each snapshot, and should include these maps in the “decb” file.<br />

Layout. <strong>BAT</strong> gain/offset map. EXTNAME = ‘Gain Offset Map’

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!