Search for broad gamma ray lines with the UCR double Compton scatter telescope

Details Search for broad gamma ray lines with the UCR double Compton scatter telescope Search for broad gamma ray lines with the UCR double Compton scatter telescope

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978grsa.rept..217w&link_type=abstract

In NASA. Goddard Space Flight Center Gamma Ray Spectry. in Astrophys. p 217-222 (SEE N78-31971 22-88)

Other

Compton Effect, Emission Spectra, Flux (Rate), Gamma Ray Telescopes, Line Spectra, Scatterometers, Spectral Line Width, Continuous Spectra, Crab Nebula, Energy Distribution, Graphs (Charts), Monte Carlo Method, Scintillation Counters

Scientific paper

The operation of a double scatter telescope and the evaluation of data obtained during a 24 hour balloon flight are discussed. An increase in gamma rays was observed as the galactic anti-center crossed the aperature of the telescope. Searches for lines from p(n,gamma)d at 2.2 MeV, C-12* at 4.4 MeV and on -16* at 6.1 MeV and for other lines broadened or redshifted are being conducted to identify the processes responsible for the production of celestial gamma rays. Two upper limits for lines in the angalactic anti-center direction at 4.4 MeV and 6.1 MeV are 6 and 4 x 10 to the minus 4 power gamma/sq cm-s.

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