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          Institute: MPI für Physik     Collection: MPI für Physik     Display Documents



ID: 544617.0, MPI für Physik / MPI für Physik
Multiwavelength observation from radio through very-high-energy Gamma-ray of OJ 287 during the 12-year cycle flare in 2007
Authors:Hayashida, M.; Bonnoli, G.; Stamerra, A.; Lindfors, E.; Nilsson, K.; Teshima, M.; Seta, H.; Isobe, N.; Tashiro, M. S.; Nakanishi, K.; Sasada, M.; Shimajiri, Y.; Uemura, M.
Audience:Not Specified
Intended Educational Use:No
Abstract / Description:We performed simultaneous multiwavelength observations of OJ 287 with the Nobeyama Millimeter Array for radio, the KANATA telescope and the KVA telescope for optical, the Suzaku satellite for X-ray and the MAGIC telescope for very high energy (VHE) gamma-ray in 2007. The observations were conducted for a quiescent state in April and in a flaring state in November-December. We clearly observed increase of fluxes from radio to X-ray bands during the flaring state while MAGIC could not detect significant VHE gamma-ray emission from the source. We could derive an upper limit (95% confidence level) of 1.7% of the Crab Nebula flux above 150 GeV from about 41.2 hours of the MAGIC observation. A simple SSC model suggests that the observed flaring activity could be caused by evolutions in the distribution of the electron population rather than changes of the magnetic field strength or Doppler beaming factor in the jet.
Classification / Thesaurus:MAGIC
Comment of the Author/Creator:Contribution to the 31st ICRC, Lodz, Poland, July 2009
Document Type:Conference-Paper
Communicated by:N.N.
Affiliations:MPI für Physik
Identifiers:LOCALID:MPP-2009-126
URL:http://www.slac.stanford.edu/spires/find/hep/www?r...
URL:http://arXiv.org/abs/arxiv:0907.1343
URL:http://publications.mppmu.mpg.de/?action=search&mp...
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