The Preliminary Cosmic Diffuse gamma -Ray Spectrum from 800 keV to 30 MeV Measured with COMPTEL

Details The Preliminary Cosmic Diffuse gamma -Ray Spectrum from 800 keV to 30 MeV Measured with COMPTEL The Preliminary Cosmic Diffuse gamma -Ray Spectrum from 800 keV to 30 MeV Measured with COMPTEL

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.5801k&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #58.01; Bulletin of the American Astronomical Society, Vol. 27, p.1368

Astronomy and Astrophysics

Astronomy

Scientific paper

We report a preliminary Cosmic Diffuse gamma -ray (CDG) spectrum from 800 keV to 30 MeV obtained with the COMPTEL instrument, the Imaging Compton Telescope on-board the Compton Gamma Ray Observatory. The spectrum is constructed by measuring the count rate of gamma rays from high galactic latitudes and first extrapolating the rate to a zero cosmic-ray flux environment to eliminate the prompt background. The prompt background is produced primarily by the interactions of protons and neutrons with the spacecraft. Second, this rate is then corrected for the effects of delayed internal radioactivity to arrive at the gamma -ray count rate due to the CDG radiation. The preliminary measurements of the CDG flux in the 2--10 MeV range is 5--10 times lower than earlier reports. The 2--30 MeV flux is consistent with power-law extrapolations from lower and higher energies. The preliminary measurements show no evidence of a `MeV bump' above 2 MeV. The bump, if present, is restricted to energies less than ~ 2 MeV\@.

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