IBIS detectability of the hard X-ray tailed sample of Bursters

Details IBIS detectability of the hard X-ray tailed sample of Bursters IBIS detectability of the hard X-ray tailed sample of Bursters

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..698b&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 698-702 (2000).

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X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

During the 2.5 years of Galactic Bulge Monitoring with the WFC on board the Beppo-SAX satellite new X-Ray Burst sources have been discovered. Some of these sources have also been promptly observed on a wide energy band by using the Narrow Field Instruments of the Satellite and a high energy component up to 200 keV has been detected. Moreover bursts behavior has been discovered with the WFC for 4 more sources previously observed with other high energy instruments enlarging the sample of studied objects. These results support the existence of such a class of previously suggested hard X-ray emitters that are very promising for the future IBIS/INTEGRAL CORE Program observations (Galactic Plane Survey and the Galactic Center Deep Exposure). Simulation results on the IBIS view on this class of object will be presented. .

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