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A search for flaring very-high-energy cosmic γ-ray sources with the L3+C muon spectrometer

  • The L3 Collaboration
  • University of Geneva
  • University of Florence
  • CIEMAT
  • Radboud University Nijmegen
  • University of Lausanne
  • CERN
  • National Institute for Nuclear Physics
  • Swiss Federal Institute of Technology Zurich
  • Louisiana State University
  • Petersburg Nuclear Physics InstituteGatchina
  • Alikhanov Institute for Theoretical and Experimental Physics
  • University of Michigan, Ann Arbor
  • Tata Institute of Fundamental Research
  • University of Rome La Sapienza
  • Florida Institute of Technology
  • German Electron Synchrotron
  • University of Amsterdam
  • Université Savoie Mont Blanc
  • Paul Scherrer Institute
  • Purdue University
  • University of Perugia
  • Massachusetts Institute of Technology
  • Carnegie Mellon University
  • RWTH Aachen University
  • Hungarian Academy of Sciences

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

The L3+C muon detector at the CERN electron-positron collider, LEP, is used for the detection of very-high-energy cosmic γ-ray sources through the observation of muons of energies above 20, 30, 50 and 100 GeV. Daily or monthly excesses in the rate of single-muon events pointing to some particular direction in the sky are searched for. The periods from mid July to November 1999, and April to November 2000 are considered. Special attention is also given to a selection of known γ-ray sources. No statistically significant excess is observed for any direction or any particular source.

Original languageEnglish
Pages (from-to)298-310
Number of pages13
JournalAstroparticle Physics
Volume25
Issue number5
DOIs
StatePublished - Jun 1 2006

Keywords

  • Gamma-ray-point-sources
  • L3+C
  • Muons

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