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The PAMELA experiment and antimatter in the universe, , , , , , , , , and 52 other author(s). Hyperfine Interactions, 228 (1): 101--109 (Oct 1, 2014)THE DISCOVERY OF GEOMAGNETICALLY TRAPPED COSMIC-RAY ANTIPROTONS, , , , , , , , , and 54 other author(s). The Astrophysical Journal, 737 (2): L29 (July 2011)PAMELA and indirect dark matter searches, , , , , , , , , and 46 other author(s). New Journal of Physics, 11 (10): 105023 (October 2009)The cosmic-ray positron energy spectrum measured by PAMELA, , , , , , , , , and 56 other author(s). (2013)cite arxiv:1308.0133Comment: 14 pages, 4 figures, 1 table. Accepted for publication in Physical Review Letters.An anomalous positron abundance in cosmic rays with energies 1.5–100 GeV, , , , , , , , , and 41 other author(s). Nature, (April 2009)MEASUREMENT OF THE ISOTOPIC COMPOSITION OF HYDROGEN AND HELIUM NUCLEI IN COSMIC RAYS WITH THE PAMELA EXPERIMENT, , , , , , , , , and 52 other author(s). The Astrophysical Journal, 770 (1): 2 (May 2013)TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THEPAMELAEXPERIMENT, , , , , , , , , and 51 other author(s). The Astrophysical Journal, 799 (1): L4 (January 2015)Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment, , , , , , , , , and 58 other author(s). JETP Letters, 96 (10): 621--627 (Jan 1, 2013)New Measurement of the Antiproton-to-Proton Flux Ratio up to 100 GeV in the Cosmic Radiation, , , , , , , , , and 43 other author(s). Phys. Rev. Lett., 102 (5): 051101 (February 2009)Observation of an anomalous positron abundance in the cosmic radiation, , , , , , , , , and 41 other author(s). (2008)cite arxiv:0810.4995 Comment: Submitted to Nature, 20 pages, 5 figures, 1 table.