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Detection of multi-TeV emission from Markarian 421

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/304090· OSTI ID:628693
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  1. Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011-3160 (United States)
  2. Randall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan 48109-1120 (United States)
  3. Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, P.O. Box 97, Amado, Arizona 85645-0097 (United States)
  4. Department of Physics, University of Leeds, Leeds, LS2 9JT, Yorkshire, England (United Kingdom)
  5. Physics Department, St. Patricks College, Maynooth, County Kildare (Ireland)
  6. Physics Department, University College, Dublin 4 (Ireland)
  7. Department of Physics, Purdue University, West Lafayette, Indiana 47907 (United States)
Gamma rays with energies exceeding 5{plus_minus}1.5TeV have been detected from Markarian 421 using the Whipple Observatory{close_quote}s 10 m {gamma}-ray telescope. These observations employ a new technique: the so-called large zenith-angle technique. Because they are taken at large zenith angles, the observations yield high statistics data on the multi-TeV part of the spectrum and are well suited for examining the question of a possible energy cutoff. Observations taken during high states on 1995 June 20, 21, and 28 show no evidence for a spectral break. These results conflict with a previous interpretation of the Markarian 421 energy spectrum in which a cutoff due to {gamma}-ray absorption in extragalactic space was postulated. {copyright} {ital 1997} {ital The American Astronomical Society}
OSTI ID:
628693
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 481; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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