Cutoff in the tev energy spectrum of markarian 421 during strong flares in 2001

F. Krennrich, H. M. Badran, I. H. Bond, S. M. Bradbury, J. H. Buckley, D. A. Carter-Lewis, M. Catanese, W. Cui, S. Dunlea, D. Das, I. Dela Calle Perez, D. J. Fegan, S. J. Fegan, J. P. Finley, J. A. Gaidos, K. Gibbs, G. H. Gillanders, T. A. Hall, A. M. Hillas, J. HolderD. Horan, M. Jordan, M. Kertzman, D. Kieda, J. Kildea, J. Knapp, K. Kosack, M. J. Lang, S. LeBohec, B. McKernan, P. Moriarty, D. Muller, R. Ong, R. Pallassini, D. Petry, J. Quinn, N. W. Reay, P. T. Reynolds, H. J. Rose, G. H. Sembroski, R. Sidwell, N. Stanton, S. P. Swordy, V. V. Vassiliev, S. P. Wakely, T. C. Weekes

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Abstract

Exceptionally strong and long-lasting flaring activity of the blazar Mrk 421 occurred between 2001 January and March. Based on the excellent signal-to-noise ratio of the data, we derive the energy spectrum between 260 GeV and 17 TeV with unprecedented statistical precision. The spectrum is not well described by a simple power law even with a curvature term. Instead, the data can be described by a power law with exponential cutoff: DN/dE ∝ E-2.14±0.03statℓ-E/E0m-2S-2 TeV-1 with E0=4.3±0.3statTeV.Mrk 421 is the second -ray blazar that 0 stat unambiguously exhibits an absorption-like feature in its spectral energy distribution at 3-6 TeV.

Original languageEnglish
Pages (from-to)L45-L48
JournalAstrophysical Journal Letters
Volume560
Issue number1
DOIs
StatePublished - Oct 10 2001

Keywords

  • BL Lacertae Objects: Individual (Markarian 421)-Gamma Rays: Observations

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