A. Taylor, G. Giacinti, P. Desiati, J. C. Vélez, A. Chiavassa, G. Sciascio, J. Velazquez, S. Kunwar
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引用次数: 2
摘要
DESY, Platanenallee 6, 15738 Zeuthen，德国MPIK, Saupfercheckweg 1, 69117 Heidelberg，德国威斯康星州麦迪逊大学，222 W。华盛顿Ave .麦迪逊,53703、U。S。A .物理系,universita degli Studi di,都灵,意大利国家核物理研究所,罗马Tor Vergata科、科学研究的道路上1、00133罗马,意大利5物理研究所和服装,大学Michoacana de Morelia Nicol as德伊达尔戈(aung San suu kyi)墨西哥电子邮件:安德鲁·taylor@desy . de Gwenael Giacinti@mpi-hd mpg。德。
Composition Sensitivity for the Cosmic Ray Anisotropy with SWGO
DESY, Platanenallee 6, 15738 Zeuthen, Germany MPIK, Saupfercheckweg 1, 69117 Heidelberg, Germany WIPAC, University of Wisconsin Madison, 222 W. Washington Ave. Madison, WI 53703, U.S.A. Dipartimento di Fisica, Università degli Studi di Torino, Torino, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, via della Ricerca Scientifica 1, 00133 Roma, Italy 5 Institute of Physics and Mathematics, Universidad Michoacana de San Nicol as de Hidalgo, Morelia, Mexico E-mail: andrew.taylor@desy.de, Gwenael.Giacinti@mpi-hd.mpg.de
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