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dc.contributor.authorAmbrosi, G.
dc.contributor.authorAzzarello, P.
dc.contributor.authorBattiston, R.
dc.contributor.authorBazo, J.
dc.contributor.authorBertucci, B.
dc.contributor.authorChoumilov, E.
dc.contributor.authorChoutko, V.
dc.contributor.authorCrispoltoni, M.
dc.contributor.authorDelgado, C.
dc.contributor.authorDuranti, M.
dc.contributor.authorDonnini, F.
dc.contributor.authorD'Urso, D.
dc.contributor.authorFiandrini, E.
dc.contributor.authorFormato, V.
dc.contributor.authorGraziani, M.
dc.contributor.authorHabiby, M.
dc.contributor.authorHaino, S.
dc.contributor.authorIonica, M.
dc.contributor.authorKanishchev, K.
dc.contributor.authorNozzoli, F.
dc.contributor.authorOliva, A.
dc.contributor.authorPaniccia, M.
dc.contributor.authorPizzolotto, C.
dc.contributor.authorPohl, M.
dc.contributor.authorQin, X.
dc.contributor.authorRapin, D.
dc.contributor.authorSaouter, P.
dc.contributor.authorTomassetti, N.
dc.contributor.authorVitale, V.
dc.contributor.authorVitillo, S.
dc.contributor.authorWu, X.
dc.contributor.authorZhang, Z.
dc.contributor.authorZuccon, P.
dc.date.accessioned2021-11-04T20:23:10Z
dc.date.available2021-11-04T20:23:10Z
dc.date.issued2015
dc.identifier.urihttps://hdl.handle.net/1721.1/137413
dc.description.abstractThe Alpha Magnetic Spectrometer (AMS-02) is an astroparticle physics detector that has been installed on the International Space Station (ISS) in May 2011. The purpose of the experiment is to study with unprecedented precision and statistics cosmic-ray particles in an energy range from 0.5 GeV to few TeV. The AMS-02 Tracker system accurately determines the trajectory and absolute charge (Z) of cosmic rays by multiple measurements of the coordinates in nine layers of double-sided silicon micro-strip detectors. Given the high dynamic range of the front-end electronics, nuclei from hydrogen up to iron and above can be identified. The charge resolution could be naturally degraded by a number of detector effects that need to be carefully accounted for. In this contribution we describe the procedure that has been used to accurately calibrate the Tracker response. Finally we will discuss the Tracker calibration stability with time.en_US
dc.language.isoen
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourceProceedings of Scienceen_US
dc.titleNuclei charge measurement with the AMS-02 silicon trackeren_US
dc.typeArticleen_US
dc.identifier.citationAmbrosi, G., Azzarello, P., Battiston, R., Bazo, J., Bertucci, B. et al. 2015. "Nuclei charge measurement with the AMS-02 silicon tracker."
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Science
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2019-05-13T11:56:18Z
dspace.date.submission2019-05-13T11:56:21Z
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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