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Multiwavelength observations of markarian 421 in 2005-2006

  • D. Horan
  • , V. A. Acciari
  • , S. M. Bradbury
  • , J. H. Buckley
  • , V. Bugaev
  • , K. L. Byrum
  • , A. Cannon
  • , O. Celik
  • , A. Cesarini
  • , Y. C.K. Chow
  • , L. Ciupik
  • , P. Cogan
  • , A. D. Falcone
  • , S. J. Fegan
  • , J. P. Finley
  • , P. Fortin
  • , L. F. Fortson
  • , D. Gall
  • , G. H. Gillanders
  • , J. Grube
  • G. Gyuk, D. Hanna, E. Hays, M. Kertzman, J. Kildea, A. Konopelko, H. Krawczynski, F. Krennrich, M. J. Lang, K. Lee, P. Moriarty, T. Nagai, J. Niemiec, R. A. Ong, J. S. Perkins, M. Pohl, J. Quinn, P. T. Reynolds, H. J. Rose, G. H. Sembroski, A. W. Smith, D. Steele, S. P. Swordy, J. A. Toner, V. V. Vassiliev, S. P. Wakely, T. C. Weekes, R. J. White, D. A. Williams, M. D. Wood, B. Zitzer, H. D. Aller, M. F. Aller, M. Baker, D. Barnaby, M. T. Carini, P. Charlot, J. P. Dumm, N. E. Fields, T. Hovatta, B. Jordan, Y. A. Kovalev, Y. Y. Kovalev, H. A. Krimm, O. M. Kurtanidze, A. L. Ahteenmaki, J. F.Le Campion, J. Maune, T. Montaruli, A. C. Sadun, S. Smith, M. Tornikoski, M. Turunen, R. Walters
  • Argonne National Laboratory
  • Galway-Mayo Institute of Technology
  • Center for Astrophysics | Harvard & Smithsonian
  • University of Leeds
  • Washington University in St. Louis
  • University College Dublin
  • University of California, Los Angeles
  • IDA Business Park
  • Adler Planetarium
  • McGill University
  • Pennsylvania State University
  • Purdue University
  • Barnard College
  • University of Chicago
  • NASA Goddard Space Flight Center
  • DePauw University
  • Pittsburg State University
  • Iowa State University
  • Institute for Nuclear Physics
  • Cork Institute of Technology
  • University of California, Santa Cruz
  • University of Michigan, Ann Arbor
  • University of Wisconsin-Madison
  • Western Kentucky University
  • Observatoire Aquitain des Sciences de L'Univers
  • Laboratoire d'Astrophysique de Bordeaux
  • Aalto University
  • Dublin Institute for Advanced Studies
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • Max-Planck-Institut für Radioastronomie
  • Universities Space Research Association
  • Abastumani Astrophysical Observatory
  • University of Colorado at Denver

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Since 2005 September, the Whipple 10 m Gamma-ray Telescope has been operated primarily as a blazar monitor. The five northern hemisphere blazars that have already been detected at the Whipple Observatory, Markarian 421 (Mrk 421), H1426+428, Mrk 501, 1ES 1959+650, and 1ES 2344+514, are monitored routinely each night that they are visible. We report on the Mrk 421 observations taken from 2005 November to 2006 June in the gamma-ray, X-ray, optical, and radio bands. During this time, Mrk 421 was found to be variable at all wavelengths probed. Both the variability and the correlations among different energy regimes are studied in detail here. A tentative correlation, with large spread, was measured between the X-ray and gamma-ray bands, while no clear correlation was evident among the other energy bands. In addition to this, the well-sampled spectral energy distribution of Mrk 421 (1101+384) is presented for three different activity levels. The observations of the other blazar targets will be reported separately.

langue originaleAnglais
Pages (de - à)596-618
Nombre de pages23
journalAstrophysical Journal
Volume695
Numéro de publication1
Les DOIs
étatPublié - 10 avr. 2009
Modification externeOui

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