PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy

Adriani, O;Barbarino, GC;Bazilevskaya, GA;Bellotti, R;Boezio, M;Bogomolov, EA;Bonechi, L;Bongi, M;Bonvicini, V;Borisov, S;Bottai, S;Bruno, A;Cafagna, F;Campana, D;Carbone, R;Carlson, P;Casolino, M;Castellini, G;Consiglio, L;DE PASCALE, MARIA PIA;DE SANTIS, CRISTIAN;De Simone, ND;De Felice, VD;Galper, AM;Gillard, W;Grishantseva, L;Hofverberg, P;Jerse, G;Karelin, AV;Koldashov, SV;Krutkov, SY;Kvashnin, AN;Leonov, A;MALVEZZI, VALERIA;Marcelli, L;Mayorov, AG;Menn, W;Mikhailov, VV;MINORI, MAURO;Mocchiutti, E;Monaco, A;Mori, N;Nikonov, N;Osteria, G;Papini, P;Pearce, M;PICOZZA, PIERGIORGIO;Pizzolotto, C;Ricci, M;Ricciarini, SB;Rossetto, L;Simon, M;SPARVOLI, ROBERTA;Spillantini, P;Stozhkov, YI;Taddei, E;Vacchi, A;Vannuccini, E;Vasilyev, G;Voronov, SA;Wu, J;Yurkin, YT;Zampa, G;Zampa, N;Zverev, VG

2010-01-01