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Simultaneous X-ray and TeV observations of a rapid flare from markarian 421

  • L. Maraschi
  • , G. Fossati
  • , F. Tavecchio
  • , L. Chiappetti
  • , A. Celotti
  • , G. Ghisellini
  • , P. Grandi
  • , E. Pian
  • , G. Tagliaferri
  • , A. Treves
  • , A. C. Breslin
  • , J. H. Buckley
  • , D. A. Carter-Lewis
  • , M. Catanese
  • , M. F. Cawley
  • , D. J. Fegan
  • , S. J. Fegan
  • , J. P. Finley
  • , J. A. Gaidos
  • , Anthony Hall
  • A. M. Hillas, F. Krennrich, R. W. Lessard, Claire Masterson, Patrick Moriarty, J. Quinn, J. Rose, F. W. Samuelson, T. C. Weekes, C. M. Urry, T. Takahashi

Research output: Contribution to a Journal (Peer & Non Peer)Articlepeer-review

Abstract

Mrk 421 was observed for about 2 days with BeppoSAX in 1998 April as part of a worldwide multiwavelength campaign. A large, well-defined flare was observed in X-rays. The same flare was observed simultaneously at TeV energies by the Whipple Observatory gamma-ray telescope. These data provide (1) the first evidence that the X-ray and TeV intensities are well correlated on timescales of hours and (2) the first exactly simultaneous X-ray and TeV spectra. The results imply that the X-ray and TeV photons derive from the same region and from the same population of relativistic electrons. The physical parameters deduced from a homogeneous synchrotron self-Compton model for the spectral energy distribution yield electron cooling times close to the observed variability timescales.
Original languageEnglish (Ireland)
Number of pages4
JournalAstrophysical Journal
Volume526
DOIs
Publication statusPublished - 1 Dec 1999

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