Next generation ground-based gamma-ray telescope

Details Next generation ground-based gamma-ray telescope Next generation ground-based gamma-ray telescope

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996spie.2806...64a&link_type=abstract

Proc. SPIE Vol. 2806, p. 64-73, Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions, Brian D. Ramsey; Thomas A. Parnell

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Scientific paper

The design of a ground based gamma ray telescope is presented. This telescope would be sensitive to extraterrestrial gamma rays with energies from 20 GeV to over 1000 GeV. Among other things, this telescope would be able to make improved studies of the emission mechanism of gamma rays from active galactic nuclei (AGNs), and of the interactions of gamma rays from AGNs with the intergalactic infrared radiation field (IIRF). When combined with independent measurements of the Hubble constant, these observations will enable the measurement of the IIRF.

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