GRIS Measurement of the Cosmic Diffuse Background Spectrum

Details GRIS Measurement of the Cosmic Diffuse Background Spectrum GRIS Measurement of the Cosmic Diffuse Background Spectrum

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...18910109b&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #101.09; Bulletin of the American Astronomical Society, Vol. 28, p.1410

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The GRIS instrument recently made a measurement of the Cosmic Diffuse spectrum during a 32 hour balloon flight from Alice Springs, Australia during 24-26 Oct 1996. A new wide- FOV configuration (100x75deg) of the GRIS instrument with a blocking crystal was used. Upper limits on steps in the spectrum at 847 and 1238 keV due to the integrated contributions of Co-56 from supernovae throughout the universe as predicted by Zdziaski (MNRS, 281, 96) and The et al.(ApJ, 403, 93) will be presented.

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