TeV observations of Markarian 501 with the Milagrito water cerenkov detector

  • R. Atkins
  • , W. Benbow
  • , D. Berley
  • , M. L. Chen
  • , D. G. Coyne
  • , R. S. Delay
  • , B. L. Dingus
  • , D. E. Dorfan
  • , R. W. Ellsworth
  • , C. Espinoza
  • , D. Evans
  • , A. Falcone
  • , L. Fleysher
  • , R. Pleysher
  • , G. Gisler
  • , J. A. Goodman
  • , T. J. Haines
  • , C. M. Hoffman
  • , S. Hugenberger
  • , L. A. Kelley
  • I. Leonor, M. McConnell, J. F. McCullough, J. E. McEnery, R. S. Miller, A. I. Mincer, M. F. Morales, M. M. Murray, P. Nemethy, J. M. Ryan, M. Schneider, B. Shen, A. Shoup, C. Sinnis, A. J. Smith, G. W. Sullivan, T. N. Thompson, T. Tumer, K. Wang, M. O. Wascko, S. Westerhoff, D. A. Williams, T. Yang, G. B. Yodh

Research output: Contribution to journalArticlepeer-review

Abstract

The Milagrito water Cerenkov detector near Los Alamos, New Mexico, was operated as a sky monitor at energies of a few TeV between 1997 February and 1998 May, including the period of the strong, long-lasting 1997 flare of Markarian 501. Milagrito served as a test run for the full Milagro detector. An event excess with a significance of 3.7 σ from Markarian 501 was observed, in agreement with expectations.

Original languageEnglish (US)
Pages (from-to)L25-L28
JournalAstrophysical Journal
Volume525
Issue number1 PART 2
DOIs
StatePublished - Nov 1 1999

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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