Detection of the BL Lac Object H1426+428 at TeV Gamma Ray Energies

نویسندگان

  • D. Horan
  • H. M. Badran
  • D. J. Fegan
  • S. J. Fegan
چکیده

Fred Lawrence Whipple Observatory, Harvard-Smithsonian CfA, P.O. Box 97, Amado, AZ 85645 Experimental Physics Department, National University of Ireland, Belfield, Dublin 4, Ireland Department of Physics, University of Leeds, Leeds, LS2 9JT, Yorkshire, England, UK Department of Physics, Washington University, St. Louis, MO 63130 Department of Physics and Astronomy, Iowa State University, Ames, IA 50011 Department of Physics, Purdue University, West Lafayette, IN 47907 Physics Department, Tanta University, Tanta, Egypt Department of Physics, University of Arizona, Tucson, AZ 85721 Physics Department, National University of Ireland, Galway, Ireland Enrico Fermi Institute, University of Chicago, Chicago, IL 60637 High Energy Astrophysics Institute, University of Utah, Salt Lake City, UT 84112 Department of Physics, University of California, Los Angeles, CA 90095 School of Science, Galway-Mayo Institute of Technology, Galway, Ireland Department of Physics, Cork Institute of Technology, Cork, Ireland Department of Physics, Kansas State University, Manhattan, KS 66506 Department of Physics and Astronomy, DePauw University, Greencastle, IN 46135 Physics & Astronomy Department, University of Arkansas at Little Rock, Little Rock, AR 72204

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X-ray spectral variability of extreme BL Lacertae active galactic nucleus H1426+428

Between 2002 March 7 and 2002 June 15, intensive X-ray observations were carried out on the extreme BL Lac object H1426+428 with instruments on board the Rossi X-Ray Timing Explorer (RXTE). These instruments provide measurements of H1426+428 in the crucial energy range that characterizes the first peak of its spectral energy distribution. This peak, which is almost certainly due to synchrotron ...

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For High frequency BL Lac objects (HBLs) like H1426+428, a significant fraction of their TeV gammarays emitted are likely to be absorbed in interactions with the diffuse IR background, yielding e pairs. The resulting e pairs generate one hitherto undiscovered GeV emission by inverse Compton scattering with the cosmic microwave background photons (CMBPs). We study such emission by taking the 199...

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تاریخ انتشار 2009