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High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station
The Alpha Magnetic Spectrometer (AMS) is a large acceptance, superconducting magnetic spectrometer designed to search for anti- matter and to study, with high accuracy, the origin of dark-matter and the composition of cosmic rays. The results of a Monte Carlo simulation study of AMS as a high-energy...
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Lenguaje: | eng |
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2002
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Acceso en línea: | https://dx.doi.org/10.1016/S0920-5632(02)01839-X http://cds.cern.ch/record/623653 |
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author | Lamanna, G |
author_facet | Lamanna, G |
author_sort | Lamanna, G |
collection | CERN |
description | The Alpha Magnetic Spectrometer (AMS) is a large acceptance, superconducting magnetic spectrometer designed to search for anti- matter and to study, with high accuracy, the origin of dark-matter and the composition of cosmic rays. The results of a Monte Carlo simulation study of AMS as a high-energy gamma -ray detector are presented. AMS will be able to provide accurate measurements of gamma -ray spectra over a broad energy range (up to hundreds of GeV) with energy resolution of a few per cent and angular resolution of 0.018-1 degrees . The acceptance of 0.04-0.13 m/sup 2/ sr has been estimated with maximal opening angle being 20 degrees to 42 degrees . The study of the background events has been done, the irreducible background- to-signal ratio being at the level of a few per cent or below being. The gamma -ray sky survey sensitivity of AMS is finally discussed. (14 refs). |
id | cern-623653 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2002 |
record_format | invenio |
spelling | cern-6236532019-09-30T06:29:59Zdoi:10.1016/S0920-5632(02)01839-Xhttp://cds.cern.ch/record/623653engLamanna, GHigh-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space StationAstrophysics and AstronomyThe Alpha Magnetic Spectrometer (AMS) is a large acceptance, superconducting magnetic spectrometer designed to search for anti- matter and to study, with high accuracy, the origin of dark-matter and the composition of cosmic rays. The results of a Monte Carlo simulation study of AMS as a high-energy gamma -ray detector are presented. AMS will be able to provide accurate measurements of gamma -ray spectra over a broad energy range (up to hundreds of GeV) with energy resolution of a few per cent and angular resolution of 0.018-1 degrees . The acceptance of 0.04-0.13 m/sup 2/ sr has been estimated with maximal opening angle being 20 degrees to 42 degrees . The study of the background events has been done, the irreducible background- to-signal ratio being at the level of a few per cent or below being. The gamma -ray sky survey sensitivity of AMS is finally discussed. (14 refs).oai:cds.cern.ch:6236532002 |
spellingShingle | Astrophysics and Astronomy Lamanna, G High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title | High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title_full | High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title_fullStr | High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title_full_unstemmed | High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title_short | High-energy gamma-ray detection with the Alpha Magnetic Spectrometer on board the International Space Station |
title_sort | high-energy gamma-ray detection with the alpha magnetic spectrometer on board the international space station |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1016/S0920-5632(02)01839-X http://cds.cern.ch/record/623653 |
work_keys_str_mv | AT lamannag highenergygammaraydetectionwiththealphamagneticspectrometeronboardtheinternationalspacestation |