An anomalous positron abundance in cosmic rays with energies 1.5–100 GeVO. Adriani, N. Zampa, N. De Simone et al.|Nature|2009Cited by 2.2k
New Measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic RadiationO. Adriani, Y. T. Yurkin, G. C. Barbarino et al.|Physical Review Letters|2009Cited by 549
PAMELA – A payload for antimatter matter exploration and light-nuclei astrophysicsP. Picozza, R. Sparvoli, A. M. Galper et al.|Astroparticle Physics|2006Cited by 433
TIME DEPENDENCE OF THE PROTON FLUX MEASURED BY PAMELA DURING THE 2006 JULY-2009 DECEMBER SOLAR MINIMUMO. Adriani, M. Simon, G. C. Barbarino et al.|The Astrophysical Journal|2013Cited by 278
MEASUREMENT OF THE ISOTOPIC COMPOSITION OF HYDROGEN AND HELIUM NUCLEI IN COSMIC RAYS WITH THE PAMELA EXPERIMENTO. Adriani, M. Simon, G. C. Barbarino et al.|The Astrophysical Journal|2013Cited by 51