Milagrito Detection of TeV Emission from Mrk 501
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Milagrito Detection of TeV Emission from Mrk 501

  • Author(s): Atkins, R
  • Benbow, W
  • Berley, D
  • Chen, M-L
  • Coyne, DG
  • Delay, RS
  • Dingus, BL
  • Dorfan, DE
  • Ellsworth, RW
  • Evans, D
  • Falcone, A
  • Fleysher, L
  • Fleysher, R
  • Gisler, G
  • Goodman, JA
  • Haines, TJ
  • Hoffman, CM
  • Hugenberger, S
  • Kelley, LA
  • Leonor, I
  • Macri, J
  • McConnell, M
  • McCullough, JF
  • McEnery, JE
  • Miller, RS
  • Mincer, AI
  • Morales, MF
  • Nemethy, P
  • Ryan, JM
  • Schneider, M
  • Shen, B
  • Shoup, A
  • Sinnis, G
  • Smith, AJ
  • Sullivan, GW
  • Thompson, TN
  • Tumer, OT
  • Wang, K
  • Wascko, MO
  • Westerhoff, S
  • Williams, DA
  • Yang, T
  • Yodh, GB
  • et al.
Abstract

The Milagro water Cherenkov detector near Los Alamos, New Mexico, has been operated as a sky monitor at energies of a few TeV between February 1997 and April 1998. Serving as a test run for the full Milagro detector, Milagrito has taken data during the strong and long-lasting 1997 flare of Mrk 501. We present results from the analysis of Mrk 501 and compare the excess and background rates with expectations from the detector simulations.

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