Particle tracking in the CALET experiment

dc.contributor.authorMaestro, Paolo
dc.contributor.authorMori, Nicola
dc.contributor.authorCannady, Nicholas
dc.contributor.authorCALET Collaboration
dc.date.accessioned2023-10-20T14:41:24Z
dc.date.available2023-10-20T14:41:24Z
dc.date.issued2018-08-03
dc.description35th International Cosmic Ray Conference — ICRC2017; Bexco, Busan, Korea; 10-20 July, 2017en_US
dc.description.abstractThe Calorimetric Electron Telescope (CALET) is a space mission installed on the Exposed Facility of the Japanese Experiment Module (JEM-EF) of the International Space Station (ISS) in August 2015 and collecting data since October 2015. In addition to high precision measurements of the electron spectrum up to TeV scale, CALET will also investigate the mechanism of cosmic-ray (CR) acceleration and propagation in the Galaxy, by performing direct measurements of the energy spectra and elemental composition of CR nuclei from H to Fe, and the abundance of trans-iron elements up to about Z=40. The instrument consists of two layers of segmented plastic scintillators to identify the particle charge, a thin (3 radiation lengths) tungsten-scintillating fiber calorimeter providing accurate particle tracking, and a thick (27 radiation lengths) calorimeter made of lead-tungstate crystal logs. In this paper we will describe an original reconstruction method of the primary particle direction based on a combinatorial Kalman filter algorithm. This method exploits the fine granularity and imaging capability of the IMC and provides robust track finding and fitting, allowing to identify the incident CR track in a large amount of shower particle tracks backscattered from the calorimeter. The track fitting algorithm has been extensively validated and tuned with simulated data. Its performance (angular resolution, impact point resolution, tracking efficiency) for electrons and nuclei will be discussed and comparisons between flight data and simulations will be shown.en_US
dc.description.sponsorshipThe CALET mission is a space experiment, funded by the Japanese AeroSpace Agency (JAXA), the Italian Space Agency (ASI) and NASA.en_US
dc.description.urihttps://pos.sissa.it/301/208/en_US
dc.format.extent8 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m21qrs-wo0r
dc.identifier.citationMaestro, Paolo, on behalf of the CALET Collaboration, and Nicola Mori. “Particle Tracking in the CALET Experiment.” In Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017), 301:208. SISSA Medialab, 2018. https://doi.org/10.22323/1.301.0208.en_US
dc.identifier.urihttps://doi.org/10.22323/1.301.0208
dc.identifier.urihttp://hdl.handle.net/11603/30306
dc.language.isoen_USen_US
dc.publisherProceedings of Scienceen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en_US
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleParticle tracking in the CALET experimenten_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-2916-6955en_US

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