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Nature|April 3, 2009
An anomalous positron abundance in cosmic rays with energies 1.5-100 GeVO Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|March 5, 2009
New measurement of the antiproton-to-proton flux ratio up to 100 GeV in the cosmic radiationO Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|July 2, 2016
Time Dependence of the Electron and Positron Components of the Cosmic Radiation Measured by the PAMELA Experiment between July 2006 and December 2015O Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|September 26, 2015
New upper limit on strange quark matter abundance in cosmic rays with the PAMELA space experimentO Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|September 28, 2010
PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energyO Adriani, G C Barbarino, G A Bazilevskaya, et al.Science (New York, N.Y.)|March 10, 2011
PAMELA measurements of cosmic-ray proton and helium spectraO Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|June 15, 2011
Cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeVO Adriani, G C Barbarino, G A Bazilevskaya, et al.Physical Review Letters|September 10, 2013
Cosmic-ray positron energy spectrum measured by PAMELAO Adriani, G C Barbarino, G A Bazilevskaya, et al.Pageof 1