Cosmic Photon and Positron Spectra Measurements Modelling with the AMS-02 Detector at ISS

Details Cosmic Photon and Positron Spectra Measurements Modelling with the AMS-02 Detector at ISS Cosmic Photon and Positron Spectra Measurements Modelling with the AMS-02 Detector at ISS

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002madm.conf..229c&link_type=abstract

MATTER, ANTI-MATTER AND DARK MATTER. Proceedings of the Second International Workshop. Held 29-30 October 2001 in Trento, Italy.

Physics

Scientific paper

The results of the MC feasibility study of the AMS-02 Detector cosmic-ray γ and e+ spectra measurement capabilities are presented. AMS will be able to provide accurate measurements of the above spectra in a broad energy range (up to hundreds of GeV) with energy resolution of a few percent and angular resolution of 0.01-1°. The acceptance of 0.05-0.15 m2sr has been estimated both for e+ and γ, with maximal opening angle being 20° to 45°. The systematic study of the background events has been done, the irreducible background to signal ratio below a few percent being obtained.

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