Detection of high-energy gamma-ray emission from the BL Lacertae object Markarian 421 by the EGRET telescope on the Compton Observatory

Y. C. Lin*, D. L. Bertsch, J. Chiang, C. E. Fichtel, R. C. Hartman, S. D. Hunter, G. Kanbach, D. A. Kniffen, P. W. Kwok, J. R. Mattox, H. A. Mayer-Hasselwander, P. F. Michelson, C. Von Montigny, P. L. Nolan, K. Pinkau, E. Schneid, P. Sreekumar, D. J. Thompson

*Corresponding author for this work

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Abstract

Gamma radiation in the energy range from 50 MeV to well over 1 GeV has been observed from the direction of the BL Lac object Markarian 421 by the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Observatory during the period 1991 June 27-July 11. The source flux is weak, but still statistically significant at the level of 10-5; the integrated photon flux above 100 MeV is (1.4 ± 0.3) × 10-7 cm-2 s-1. The differential photon energy spectrum can be represented by a power law with exponent 1.96 ± 0.14. This is the first detection of gamma-ray emission from a BL Lac object.

Original languageEnglish
Pages (from-to)L61-L64
JournalAstrophysical Journal
Volume401
Issue number2 PART 2
DOIs
Publication statusPublished - 20-12-1992

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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