CANGAROO-III OBSERVATION OF TEV GAMMA RAYS FROM THE VICINITY OF PSR B1706−44 R. Enomoto J. Kushida T. Nakamori T. Kifune

نویسندگان

  • G. V. Bicknell
  • R. W. Clay
  • P. G. Edwards
  • S. Gunji
  • S. Hara
  • T. Hara
  • T. Hattori
  • S. Hayashi
  • F. Kajino
  • H. Katagiri
  • A. Kawachi
  • R. Kiuchi
  • H. Kubo
چکیده

Observation by the CANGAROO-III stereoscopic system of the Imaging Cherenkov Telescope has detected extended emission of TeV gamma rays in the vicinity of the pulsar PSR B1706−44. The strength of the signal observed as gamma-ray-like events varies when we apply different ways of emulating background events. The reason for such uncertainties is argued in relevance to gamma-rays embedded in the “off-source data”, that is, unknown sources and diffuse emission in the Galactic plane, namely, the existence of a complex structure of TeV gamma-ray emission around PSR B1706−44. Subject headings: gamma rays: observation — pulsar: individual (PSR B1706-44) — diffuse radiation

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تاریخ انتشار 2009