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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

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5.8. MAKING <strong>BAT</strong> SKY IMAGES 47<br />

Figure 5.5: Schematic diagram of making sky images using batfftimage.<br />

5.7.11 Making Multiple Spectra<br />

By default, batbinevt makes a single (type I) pulse height spectrum. You can choose other energy<br />

binning strategies. Please see then time-selection section of the Light Curve thread for more ideas<br />

on how to do this.<br />

5.8 Making <strong>BAT</strong> Sky Images<br />

This thread describes how to make a sky image from <strong>BAT</strong> event data using the ‘batbinevt’ and<br />

‘batfftimage’ tasks.<br />

Figure 5.5 shows schematically how sky images are created using the batfftimage from detector<br />

images. Note that the sky image on the right hand side covers a significant portion of the sky (∼2<br />

steradians).<br />

5.8.1 Introduction<br />

While the <strong>BAT</strong> does not have focussing optics, it is possible to create sky images using the task<br />

batfftimage. This task combines a detector plane image and information about the coded aperture<br />

pattern to reconstruct the sky flux at each point in the field of view. Sky images have the same<br />

flux units as all other mask weighted counts values.<br />

<strong>The</strong> steps of this procedure are: (1) make a source detector plane image using batbinevt; (2)<br />

optionally make a background detector plane image; and finally (3) to make a sky image using<br />

batfftimage.<br />

5.8.2 Prerequisites<br />

• <strong>BAT</strong> event data<br />

– for example, (in obsid/bat/event/swNNNNNNNNNNNbevshsp uf.evt.gz);<br />

<strong>BAT</strong> quality map,

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