Simulation of Galactic Gamma-Ray Sources Observed with INTEGRAL/PICsIT

Details Simulation of Galactic Gamma-Ray Sources Observed with INTEGRAL/PICsIT Simulation of Galactic Gamma-Ray Sources Observed with INTEGRAL/PICsIT

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cnoc.conf...17f&link_type=abstract

The Second National Conference on Astrophysics of Compact Objects, held in Bologna (Italy), September 19 - 21, 2001, p. 17

Astronomy and Astrophysics

Astrophysics

Scientific paper

INTEGRAL is a gamma-ray observatory in the energy band 15 keV - 10 MeV scheduled for launch at the end of 2002. PICsIT is the high- energy detector (0.15 - 10 MeV) of the imager IBIS. To show the imaging capabilities of PICsIT, a software package has been developed by coupling a Montecarlo simulation code with the scientific analysis pipeline prototype. The shadowgrams and deconvolved images, obtained by simulating some galactic gamma-ray sources, are shortly discussed with reference to imaging capabilities and effectiveness of deconvolution.

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