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Details for Upper limit on the antihelium flux in primary cosmic rays
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NameUpper limit on the antihelium flux in primary cosmic rays
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Authors: A. G. Mayorov,A. M. Galper,O. Adriani,G. A. Bazilevskaya,G. Barbarino,R. Bellotti,M. Boezio,E. A. Bogomolov,V. Bonvicini,M. Bongi,L. Bonechi,S. V. Borisov,S. Bottai,A. Bruno,S. Vacci,E. Vannuccini,G. I. Vasiliev,S. A. Voronov,Y. Wu,I. A. Danilchenko,W. Gillard,G. Jerse,G. Zampa,N. Zampa,V. G. Zverev,M. Casolino,D. Campana,R. Carbone,A. V. Karelin,P. Carlson,G. Castellini,F. Cafagna,A. N. Kvashnin,S. V. Koldashov,S. A. Koldobsky,S. Yu. Krutkov,A. A. Leonov,V. V. Malakhov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,N. Mori,N. V. Nikonov,G. Osteria,S. Pizzolotto,P. Papini,M. P. Pascale,P. Picozza,M. Pearce,M. Ricci,S. Ricciarini,M. F. Runtso,M. Simon,N. Simone,R. Sparvoli,P. Spillantini,Yu. I. Stozhkov,V. Felice,Yu. T. Yurkin
Journal: JETP Letters

Volume: 93, Issue 11
Pages: 628-631
Year: 2011
DOI: 10.1134/S0021364011110087

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