Muon Astronomy with LVD Detector

Details Muon Astronomy with LVD Detector Muon Astronomy with LVD Detector

1999-05-25

arxiv.org/abs/hep-ex/9905048v1

Physics

High Energy Physics

High Energy Physics - Experiment

6 pages, 3 figures, submitted to the Proc. of 26th Intern. Cosmic Ray Conf., Salt Lake City (USA), August 17-25, 1999, SH 3.2.

Scientific paper

We analysed the arrival directions of single muons detected by the first LVD tower from November, 1994 till January, 1998. The moon shadowing effect has been observed. To search for point sources of high energy photons we have analysed muons crossing the rock thickness greater than 3, 5 and 7 km w.e., which corresponds to the mean muon energies 1.6, 3.9 and 8.4 TeV at the surface, respectively. Upper limits on steady muon fluxes for selected astrophysical sources for different muon energies are presented.

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