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

Bazzano, A.; De Cesare, G.; Cocchi, M.; Natalucci, L.; Ubertini, P.
April 2000
AIP Conference Proceedings;2000, Vol. 510 Issue 1, p698
Academic Journal
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. © 2000 American Institute of Physics.


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