A search for weak gamma-ray bursts with GRANAT/SIGMA

Astronomy and Astrophysics – Astronomy

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Gamma Ray Bursts, Gamma Ray Telescopes, Milky Way Galaxy, Spaceborne Astronomy, Galactic Nuclei, Sky Surveys (Astronomy)

Scientific paper

Results are presented of a search for weak gamma-ray bursts (GRB) with GRANAT/SIGMA, during which the narrow-aperture coded mask telescope SIGMA was operated for about 5300 hr. Despite the high sensitivity of the cell to the on-axis events, no bursts were actually found within the coded field of view. For an object located at a distance of 8.5 kpc, the threshold burst luminosity in the 40-90 keV band was found to be comparable with the Eddington limit for a neutron star. The absence of weak GRB events form the Galactic center direction indicates that either the luminosity of a typical GRB is below about 10 exp 38 ergs/sec and GRB are of local origin, or, alternatively, that the luminosity is as high as about 10 exp 40 ergs/sec or greater and most GRBs come from a massive galactic 'halo' or are of cosmological origin.

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