Detection of gamma rays with E > 300 from from markartan 501

  • J. Quinn
  • , C. W. Akerlof
  • , S. Biller
  • , J. Buckley
  • , D. A. Carter-Lewis
  • , M. F. Cawley
  • , M. Catanese
  • , V. Connaughton
  • , D. J. Fegan
  • , J. P. Finley
  • , J. Gaidos
  • , A. M. Hillas
  • , R. C. Lamb
  • , F. Krennrich
  • , R. Lessard
  • , J. E. McEnery
  • , D. I. Meyer
  • , G. Mohanty
  • , A. J. Rodgers
  • , H. J. Rose
  • M. S. Schubnell, G. Sembroski, T. C. Weekes, C. Wilson, J. Zweerink

Research output: Contribution to journalArticlepeer-review

336 Scopus citations

Abstract

The detection of gamma rays of energy greater than 300 GeV from the BL Lacertae object Mrk 501 demonstrates that extragalactic TeV emission is not unique to Mrk 421. During 66 hr of observations between 1995 March and July we measured an average flux of 8.1 ± 1.4 × 10 12 cm -2 s -1 above 300 GeV, a flux that is only 20% of the average Mrk 421 flux. The new gamma-ray source has not been reported by the Compton Gamma Ray Observatory as an emitter of gamma rays at lower energies. There is evidence for variability on timescales of days BL Lacertae.

Original languageEnglish
Pages (from-to)L83-L86
JournalAstrophysical Journal
Volume456
Issue number2
DOIs
StatePublished - Nov 1 1995

Keywords

  • Gamma rays: Observations
  • Objects: Individual (markarian 501)

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