Earth Occultation Monitoring of the Hard X-ray/Low-Energy Gamma Ray Sky with GBM

Details Earth Occultation Monitoring of the Hard X-ray/Low-Energy Gamma Ray Sky with GBM Earth Occultation Monitoring of the Hard X-ray/Low-Energy Gamma Ray Sky with GBM

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.3610c&link_type=abstract

American Astronomical Society, HEAD meeting #12, #36.10

Astronomy and Astrophysics

Astronomy

Scientific paper

By utilizing the Earth occultation technique (EOT), the Gamma-Ray Burst Monitor (GBM) instrument aboard Fermi has been used to make nearly continuous full-sky observations in the 8-1000 keV energy range. The GBM EOT analysis program currently monitors an input catalog containing 107 sources. We will present the GBM catalog of sources observed in the first 3 years of the EOT monitoring program, with special emphasis on the high energy (>100 keV) and time-variable sources, in particular the Crab and Cyg X-1. We will also describe the initial results of an all-sky imaging analysis of the EOT data, with comparisons to the Swift, INTEGRAL, and Fermi LAT catalogs. This work is supported by the NASA Fermi Guest Investigator program and NASA/Louisiana Board of Regents Cooperative Agreement NNX07AT62A.

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