Overview of TeV Gamma-Ray Observations

Details Overview of TeV Gamma-Ray Observations Overview of TeV Gamma-Ray Observations

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ssrv...75...53l&link_type=abstract

Space Science Reviews, Volume 75, Issue 1-2, pp. 53-65

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Scientific paper

TeV emission has been observed with high signal-to-noise from: two pulsar-driven supernova remnants, the Crab Nebula and PSR B1706-44 and a blazar class AGN, Markarian 421. Other sources, observed without the benefit of major background reduction techniques, are some of the compact object binaries. These discoveries plus the discoveries of EGRET of more than 130 sources at lower energies point to a growing number of scientific questions capable of being addressed by this field (particularly for distant sources via intergalactic absorption processes). Rapid further development will come as new instruments employing a variety of background reduction techniques come on-line.

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