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Cosmic-Ray Positron Identification with the PAMELA experiment

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arxiv 1306.2198 v2 pith:ECME4RNZ submitted 2013-06-10 astro-ph.HE

Cosmic-Ray Positron Identification with the PAMELA experiment

O. Adriani , G.C. Barbarino , G.A. Bazilevskaya , R. Bellotti , A. Bianco , M. Boezio , E.A. Bogomolov , M. Bongi
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V. Bonvicini S. Bottai A. Bruno F. Cafagna D. Campana R. Carbone P. Carlson M. Casolino G. Castellini C. De Santis M.P. De Pascale C. De Donato N. De Simone V. Di Felice V. Formato A.M. Galper A.V. Karelin S.V. Koldashov S. Koldobskiy S.Yu. Krut'kov A.N. Kvashnin A. Leonov V. Malakhov L. Marcelli M. Martucci A.G. Mayorov W. Menn M. Merge` V.V. Mikhailov E. Mocchiutti A. Monaco N. Mori R. Munini G. Osteria F. Palma P. Papini M. Pearce P. Picozza C. Pizzolotto M. Ricci S.B. Ricciarini L. Rossetto R. Sarkar M. Simon V. Scotti R. Sparvoli P. Spillantini S.J. Stochaj J.C. Stockton Y.I. Stozhkov A. Vacchi E. Vannuccini G. Vasilyev S.A. Voronov Y.T. Yurkin G. Zampa N. Zampa V.G. Zverev
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keywords energyexperimentpamelacosmicpositronrangerayssatellite
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The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range. One of PAMELA's main goal is the study of the antimatter component of cosmic rays. The experiment, housed on board the Russian satellite Resurs-DK1, was launched on June 15th 2006 and it is still taking data. In this work we present the measurement of galactic positron energy spectrum in the energy range between 500 MeV and few hundred GeV.

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