Observing the Soft Gamma Ray Sky - Analysis of the INTEGRAL/IBIS Galactic Plane Survey

Details Observing the Soft Gamma Ray Sky - Analysis of the INTEGRAL/IBIS Galactic Plane Survey Observing the Soft Gamma Ray Sky - Analysis of the INTEGRAL/IBIS Galactic Plane Survey

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20514208b&link_type=abstract

American Astronomical Society Meeting 205, #142.08; Bulletin of the American Astronomical Society, Vol. 36, p.1582

Astronomy and Astrophysics

Astrophysics

Scientific paper

The INTErnational Gamma Ray Astrophysical Laboratory has been in orbit for two years. In this time the survey program has concentrated on the detection of weak persistent sources in the energy range 20-100 keV. The first catalogue from the high energy (>20 keV) imager on board INTEGRAL (IBIS) was published in May 2004 and presented the location of 123 sources including 28 unidentified sources characterised by soft gamma ray emission. The general properties of these unknown sources are discussed here along with more specific analysis of a small selection of objects.

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