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Report number hep-ex/9905048
Title Muon Astronomy with LVD Detector
Author(s)

Aglietta, M ; Alyea, E D ; Antonioli, P ; Badino, G ; Bari, G ; Basile, M ; Berezinsky, Veniamin Sergeevich ; Bersani, F ; Bertaina, M ; Bertoni, R ; Bruni, G ; Cara Romeo, G ; Castagnoli, C ; Castellina, A ; Chiavassa, A ; Chinellato, J A ; Cifarelli, Luisa ; Cindolo, F ; Contin, A ; Dadykin, V L ; Dos Santos, L G ; Enikeev, R I ; Fulgione, W ; Galeotti, P ; Ghia, P ; Giusti, P ; Gómez, F ; Granella, R ; Grianti, F ; Gurentsov, V I ; Iacobucci, G ; Inoue, N ; Kemp, E ; Khalchukov, F F ; Korolkova, E V ; Korchaguin, P V ; Korchaguin, V B ; Kudryavtsev, V A ; Luvisetto, Marisa L ; Malguin, A S ; Massam, Thomas ; Mengotti-Silva, N ; Morello, C ; Nania, R ; Navarra, G ; Periale, L ; Pesci, A ; Picchi, P ; Pless, I A ; Ryasny, V G ; Ryazhskaya, O G ; Saavedra, O ; Saitoh, K ; Sartorelli, G ; Selvi, M ; Taborgna, N ; Talochkin, V P ; Trinchero, G C ; Tsuji, S ; Turtelli, A ; Vallania, P ; Vernetto, S ; Vigorito, C ; Votano, L ; Wada, T ; Weinstein, R ; Widgoff, M ; Yakushev, V F ; Yamamoto, I ; Zatsepin, G T ; Zichichi, Antonino

In: 26th International Cosmic-ray Conference, Salt Lake City, UT, USA, 17 - 25 Aug 1999, pp.e-proc, 7.SH.3.2.40
Subject category Particle Physics - Experiment
Abstract 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.

Corresponding record in: Inspire
Email contact: v.kudryavtsev@sheffield.ac.uk


 Record created 1999-05-26, last modified 2017-12-14


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