TeV gamma-ray observations of the galactic center

  • K. Kosack
  • , H. M. Badran
  • , I. H. Bond
  • , P. J. Boyle
  • , S. M. Bradbury
  • , J. H. Buckley
  • , D. A. Carter-Lewis
  • , O. Celik
  • , V. Connaughton
  • , W. Cui
  • , M. Daniel
  • , M. D'Vali
  • , I. De La Calle Perez
  • , C. Duke
  • , A. Falcone
  • , D. J. Fegan
  • , S. J. Fegan
  • , J. P. Finley
  • , L. F. Fortson
  • , J. A. Gaidos
  • S. Gammell, K. Gibbs, G. H. Gillanders, J. Grube, K. Gutierrez, J. Hall, T. A. Hall, D. Hanna, A. M. Hillas, J. Holder, D. Horan, A. Jarvis, M. Jordan, G. E. Kenny, M. Kertzman, D. Kieda, J. Kildea, J. Knapp, H. Krawczynski, F. Krennrich, M. J. Lang, S. Le Bohec, E. Linton, J. Lloyd-Evans, A. Milovanovic, J. McEnery, P. Moriarty, D. Muller, T. Nagai, S. Nolan, R. A. Ong, R. Pallassini, D. Petry, 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, V. V. Vassiliev, S. P. Wakely, G. Walker, T. C. Weekes, J. Zweerink

Research output: Contribution to journalArticlepeer-review

199 Scopus citations

Abstract

We report a possible detection of TeV gamma rays from the Galactic center by the Whipple 10 m gamma-ray telescope. Twenty-six hours of data were taken over an extended period from 1995 through 2003 resulting in a total significance of 3.7 σ. The measured excess corresponds to an integral flux of 1.6 × 10-8 ± 0.5 × 10-8 (stat) ± 0.3 × 10-8 (sys) photons m-2 s-1 above an energy of 2.8 TeV, roughly 40% of the flux from the Crab Nebula at this energy. The 95% confidence region has an angular extent of about 15′ and includes the position of Sgr A*. The detection is consistent with a point source and shows no evidence of variability.

Original languageEnglish (US)
Pages (from-to)L97-L100
JournalAstrophysical Journal
Volume608
Issue number2 II
DOIs
StatePublished - Jun 20 2004

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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