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The very high energy gamma ray spectra of IES 1959+650 and Mrk 421 as measured with the Whipple 10 m telescope

  • M. K. Daniel
  • , H. M. Badran
  • , I. H. Bond
  • , P. J. Boyle
  • , S. M. Bradbury
  • , J. H. Buckley
  • , K. Byrum
  • , D. A. Carter-Lewis
  • , O. Celik
  • , P. Cogan
  • , W. Cui
  • , I. De La Calle Perez
  • , C. Duke
  • , A. Falcone
  • , D. J. Fegan
  • , S. J. Fegan
  • , J. P. Finley
  • , L. F. Fortson
  • , S. Gammell
  • , K. Gibbs
  • G. H. Gillanders, J. Grube, K. J. Guiterrez, J. Hall, D. Hanna, J. Holder, D. Horan, S. Hughes, T. B. Humensky, I. Jung, G. E. Kenny, M. Kertzman, D. Kieda, J. Kildea, J. Knapp, K. Kosack, H. Krawczynski, F. Krennrich, M. J. Lang, S. Le Bohec, E. Linton, J. Lloyd-Evans, D. Mendoza, A. Merriman, A. Milovanovic, P. Moriarty, T. Nagai, R. A. Ong, R. Pallassini, J. Perkins, D. Petry, M. Pohl, B. Power-Mooney, J. Quinn, M. Quinn, K. Ragan, P. Rebillot, P. T. Reynolds, H. J. Rose, M. Schroedter, G. H. Sembroski, S. P. Swordy, A. Syson, L. Valcarcel, V. V. Vassiliev, R. Wagner, S. P. Wakely, G. Walker, T. C. Weekes, R. J. White, J. Zweerink
  • Iowa State University

Research output: Chapter in Book or Conference Publication/ProceedingConference Publicationpeer-review

1 Citation (Scopus)

Abstract

In observations made with the Whipple 10 m telescope, 1ES 1959+650 (z = 0.048) was caught in a high flaring state in May 2002, concurrent with a high X-ray state, and in June 2002, for which there was no corresponding X-ray flare. The spectra for both of those occasions are well fitted by a power law of differential spectral index ∼ -2.8. The relative stability of the spectral index for those flares argues strongly in favour of a two-component model as to the emission zones for the two radiation regimes. Markarian 421 (z = 0.031) was observed to be in a high flaring state, at levels of ≥ 3 Crab, during March and April 2004. The average spectrum over this time period shows evidence for a cut-off in the spectrum at ∼ 5 TeV, similar to a cut-off seen during an equivalently strong episode of flaring activity in 2001. The continued appearance of this feature indicates a long term stability, either in the physical conditions at the source, or in the intervening medium (such as attenuation on the extra-galactic infra-red background radiation).

Original languageEnglish
Title of host publicationHigh Energy Gamma-Ray Astronomy - 2nd International Symposium on High Energy Gamma-Ray Astronomy
Pages462-467
Number of pages6
DOIs
Publication statusPublished - 2005
EventInternational Symposium on High Energy Gamma-Ray Astronomy - Heidelberg, Germany
Duration: 26 Jul 200430 Jul 2004

Publication series

NameAIP Conference Proceedings
Volume745
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceInternational Symposium on High Energy Gamma-Ray Astronomy
Country/TerritoryGermany
CityHeidelberg
Period26/07/0430/07/04

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