Calculation of the gamma-ray line sensitivity of the BATSE large area detectors on GRO

Details Calculation of the gamma-ray line sensitivity of the BATSE large area detectors on GRO Calculation of the gamma-ray line sensitivity of the BATSE large area detectors on GRO

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..232..495p&link_type=abstract

Gamma-ray line astrophysics. AIP Conference Proceedings, Volume 232, pp. 495-497 (1991).

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Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables

Scientific paper

The gamma-ray line sensitivity of the BATSE detectors depends primarily upon the characteristics of the detectors' response and the nature of the backgrounds observed by the instruments. Using the example of the detectability of prompt annihilation radiation from nearby novae, the detector response characteristics and data analysis tools relevant to gamma-ray line and continuum sensitivity determination will be presented. Sensitivities to gamma-ray lines at various energies will be presented.

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