Physics
Scientific paper
Jul 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..921..296t&link_type=abstract
THE FIRST GLAST SYMPOSIUM. AIP Conference Proceedings, Volume 921, pp. 296-298 (2007).
Physics
X-Ray Sources, X-Ray Bursts, Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation
Scientific paper
Here, we consider the question of which of the 20-100 keV INTEGRAL sources may be detected by GLAST. There are clearly some source types that the two satellites will have in common, such as Active Galactic Nuclei, rotation-powered pulsars, and supernova remnants, but we have performed a detailed cross-correlation between the positions of the 499 INTEGRAL sources and the 271 EGRET sources that were detected at >100 MeV. We find that 31 of the EGRET sources have at least one INTEGRAL source in their error circle. Although source confusion is a problem in the Galactic Center region, we find 4 possible associations between EGRET sources and High-Mass X-ray Binaries in the Galactic disk. This could indicate that some fraction of HMXBs will be seen by GLAST.
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