Three years of Fermi GBM Earth Occultation Monitoring: Observations of Hard X-ray/Soft Gamma-Ray Sources
P. Jenke, Colleen A. Wilson-Hodge, Gary L. Case, Michael L. Cherry,, James Rodi, Ascension Camero-Arranz, Vandiver Chaplin, Elif Beklen, Mark H., Finger, Narayana Bhat, Michael S. Briggs, Valerie Connaughto, Jochen Greiner,, R. Marc Kippen, Charles A. Meegan, William S. Paciesas

TL;DR
This paper reports on three years of Fermi GBM Earth occultation data analysis, detecting nearly 100 high-energy sources and discussing the technique's challenges, results, and future prospects in gamma-ray astronomy.
Contribution
It presents the first three-year catalog of sources detected via Earth occultation with Fermi GBM, including methodological insights and detection of new transient sources.
Findings
Detected 99 sources, including X-ray binaries, active galaxies, and the Crab Nebula.
Identified sources in the 100-300 keV and 300-500 keV energy bands.
Enhanced detection of transient and persistent sources over three years.
Abstract
The Gamma ray Burst Monitor (GBM) on board Fermi Gamma-ray Space Telescope has been providing continuous data to the astronomical community since 2008 August 12. We will present the results of the analysis of the first three years of these continuous data using the Earth occultation technique to monitor a catalog of 209 sources. Although the occultation technique is in principle quite simple, in practice there are many complications including the dynamic instrument response, source confusion, and scattering in the Earth's atmosphere, which will be described. We detect 99 sources, including 40 low-mass X-ray binary/neutron star systems, 31 high-mass X-ray binary/neutron star systems, 12 black hole binaries, 12 active galaxies, 2 other sources, plus the Crab Nebula and the Sun. Nine of these sources are detected in the 100-300 keV band, including seven black-hole binaries, the active…
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Taxonomy
TopicsNuclear Physics and Applications · Gamma-ray bursts and supernovae · Particle Detector Development and Performance
