Performance of the first ANTARES detector line

M. Ageron, J. A. Aguilar, A. Albert, F. Ameli, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, J. J. Aubert, J. Aublin, R. Auer, S. Basa, M. Bazzotti, Y. Becherini, V. Bertin, S. Biagi, A. Bigi, C. Bigongiari, M. Bou-Cabo, M. C. BouwhuisR. Bruijn, J. Brunner, G. F. Burgio, J. Busto, F. Camarena, A. Capone, G. Carminati, J. Carr, D. Castel, E. Castorina, V. Cavasinni, S. Cecchini, Ph Charvis, T. Chiarusi, M. Circella, C. Colnard, R. Coniglione, H. Costantini, N. Cottini, P. Coyle, G. De Bonis, P. Decowski, I. Dekeyser, A. Deschamps, C. Donzaud, D. Dornic, D. Drouhin, F. Druillole, T. Eberl, J. P. Ernenwein, S. Escoffier, E. Falchini, F. Fehr, V. Flaminio, K. Fratini, J. L. Fuda, G. Giacomelli, K. Graf, G. Guillard, G. Hallewell, Y. Hello, J. J. Hernández-Rey, J. Hößl, M. de Jong, N. Kalantar-Nayestanaki, O. Kalekin, A. Kappes, U. Katz, P. Kooijman*, C. Kopper, A. Kouchner, W. Kretschmer, S. Kuch, R. Lahmann, P. Lamare, G. Lambard, H. Laschinsky, J. Lavalle, H. Le Provost, D. Lefèvre, G. Lelaizant, G. Lim, D. Lo Presti, H. Loehner, S. Loucatos, F. Louis, F. Lucarelli, K. Lyons, S. Mangano, M. Marcelin, A. Margiotta, J. A. Martinez-Mora, G. Maurin, A. Mazure, M. Melissas, E. Migneco, T. Montaruli, M. Morganti, L. Moscoso, H. Motz, C. Naumann, R. Ostasch, G. E. Pǎvǎlaş, P. Payre, J. Petrovic, C. Petta, P. Piattelli, C. Picq, R. Pillet, V. Popa, T. Pradier, E. Presani, C. Racca, A. Radu, C. Reed, C. Richardt, M. Rujoiu, M. Ruppi, G. V. Russo, F. Salesa, P. Sapienza, F. Schoeck, J. P. Schuller, R. Shanidze, F. Simeone, M. Spurio, G. van der Steenhoven, C. Tamburini, L. Tasca, S. Toscano, M. Vecchi, P. Vernin, G. Wijnker, E. de Wolf, D. Zaborov, J. D. Zornoza, J. Zúñiga


研究成果: Article査読

56 被引用数 (Scopus)


In this paper we report on the data recorded with the first Antares detector line. The line was deployed on the 14th of February 2006 and was connected to the readout 2 weeks later. Environmental data for one and a half years of running are shown. Measurements of atmospheric muons from data taken from selected runs during the first 6 months of operation are presented. Performance figures in terms of time residuals and angular resolution are given. Finally the angular distribution of atmospheric muons is presented and from this the depth profile of the muon intensity is derived.

ジャーナルAstroparticle Physics
出版ステータスPublished - 2009 5

ASJC Scopus subject areas

  • 天文学と天体物理学


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