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Results of PICsIT image analysis

In case of a staring the output images are in file

./picsit_ima.fits
For each energy range and each type of event (single, multiple), 2 types of images, INTENSITY and SIGNIFICANCE, are produced. In case PICSIT_inCorVar=1, a variance map is also produced.

The list of found sources is in the file

./picsit_sky_res.fits

In our example the Crab is the only real source that was found.

In Figure [*] you see the resulting image in the keV energy range. The Crab is clearly seen in the center. The figure was produced with the help of ds9:

cat2ds9 isgri_catalog.fits cat.reg symbol=circle color=red
ds9 picsit_ima.fits\[5] -region cat.reg \
                           -cmap cool -scale linear -scale limits 0 7 -zoom 8

Figure: Crab significance image in the keV energy band as seen by PICsIT.
Image pics_crab

In the case of observations with dithering pattern (staring=no), the pipeline performs the shadowgram deconvolution in every Science Window and the output files are under:

./scw/RRRRPPPPSSSF.001/picsit_ima.fits
./scw/RRRRPPPPSSSF.001/picsit_sky_res.fits

and the integration of all these images (mosaic) is in:

./picsit_ima.fits


next up previous contents
Next: PICsIT spectral extraction from Up: PICsIT Image Reconstruction Previous: PICsIT Image Reconstruction

2020-09-18