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The Whipple Observatory 10 m gamma-ray telescope, 1997-2006

  • J. Kildea
  • , R. W. Atkins
  • , H. M. Badran
  • , G. Blaylock
  • , I. H. Bond
  • , S. M. Bradbury
  • , J. H. Buckley
  • , D. A. Carter-Lewis
  • , O. Celik
  • , Y. C.K. Chow
  • , W. Cui
  • , P. Cogan
  • , M. K. Daniel
  • , I. de la Calle Perez
  • , C. Dowdall
  • , C. Duke
  • , A. D. Falcone
  • , D. J. Fegan
  • , S. J. Fegan
  • , J. P. Finley
  • L. F. Fortson, D. Gall, G. H. Gillanders, J. Grube, K. J. Gutierrez, J. Hall, T. A. Hall, J. Holder, D. Horan, S. B. Hughes, M. Jordan, I. Jung, G. E. Kenny, M. Kertzman, J. Knapp, A. Konopelko, K. Kosack, H. Krawczynski, F. Krennrich, M. J. Lang, S. LeBohec, J. Lloyd-Evans, J. Millis, P. Moriarty, T. Nagai, P. A. Ogden, R. A. Ong, J. S. Perkins, D. Petry, F. Pizlo, M. Pohl, J. Quinn, M. Quinn, P. F. Rebillot, H. J. Rose, M. Schroedter, G. H. Sembroski, A. W. Smith, A. Syson, J. A. Toner, L. Valcarcel, V. V. Vassiliev, S. P. Wakely, T. C. Weekes, R. J. White

Research output: Contribution to journal › Article › peer-review

Abstract

Details are presented of the Whipple Observatory's 10 m atmospheric Cherenkov telescope and camera, as it evolved during the period 1997 until 2006. The design of the telescope and camera's optical and electronic systems is discussed together with a detailed description of the four-stage GRANITE (Gamma-RAy New Imaging TElescope) upgrade program, undertaken during the same time period. The objective of the upgrade was to improve the telescope's sensitivity for the detection of very-high-energy gamma-rays. Results from the program are provided and are briefly discussed in the context of the design of VERITAS.

Original languageEnglish (US)
Pages (from-to)182-195
Number of pages14
JournalAstroparticle Physics
Volume28
Issue number2
DOIs
StatePublished - Oct 2007

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics

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