Gamma-ray variability of BL Lacs at E>300 GeV

  • J. H. Buckley
  • , C. W. Akerlof
  • , S. Biller
  • , P. J. Boyle
  • , A. C. Breslin
  • , D. A. Carter-Lewis
  • , M. Cantanese
  • , M. F. Cawley
  • , V. Connaughton
  • , D. J. Fegan
  • , J. P. Finley
  • , J. Gaidos
  • , J. Bussons Gordo
  • , A. M. Hillas
  • , F. Krennrich
  • , R. C. Lamb
  • , R. Lessard
  • , C. Masterson
  • , J. E. McEnery
  • , G. Mohanty
  • P. Moriarty, J. Quinn, A. J. Rodgers, H. J. Rose, F. Samuelson, M. S. Schubnell, G. Sembroski, R. Srinivasan, T. C. Weekes, C. Wilson, J. Zweerink

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

We report on observations of Mrk 421 and Mrk 501 at Eγ >300 GeV during the 1995 and 1996 seasons. A multiwavelength observing campaign on Mrk 421 in the period 1995 April 20 to May 5 indicates correlations in the γ-ray, X-ray, extreme ultraviolet, and optical wavelengths. Dramatic outbursts of TeV γ-rays were detected on two occasions in May of 1996 where the γ-ray flux reached the highest levels ever recorded (a factor of ∼20 greater than typical levels) with variability timescales ≲1hr. Together with the multiwavelength correlations these provide serious constraints on the Doppler factor (δ ≳ 9.9), the size and location of the emission region (R ≲ 10-4pc) and the mechanism responsible for the γ-ray emission.

Original languageEnglish
Pages (from-to)101-107
Number of pages7
JournalAdvances in Space Research
Volume21
Issue number1-2
DOIs
StatePublished - 1998

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