Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration

Autores
Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; Andreev, V.; Anzalone, A.; Arai, Y.; Asano, K.; Ave Pernas, M.; Barrillon, P.; Batsch, T.; Bayer, J.; Bechini, R.; Belenguer, T.; Bellotti, R.; Belov, K.; Berlind, A. A.; Bertaina, M.; Biermann, P. L.; Biktemerova, S.; Blaksley, C.; Blanc, N.; Blecki, J.; Blin-bondil, S.; Blumer, J.; Bobik, P.; Bogomilov, M.; Bonamente, M.; Supanitsky, Alberto Daniel; Guzman, A.; Mernik, T.; The JEM-EUSO Collaboration
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Mounted on the International Space Station(ISS), the Extreme UniverseSpace Observatory, on-board the Japanese Experimental Module (JEM-EUSO),relies on the well established fluorescence technique to observe Extensive Air Showers (EAS) developing in the earth?s atmosphere. Focusing on the detection of Ultra High Energy Cosmic Rays (UHECR) in the decade of 10 20 eV, JEM-EUSO will face new challenges by applying this technique from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed in this context to provide a full end-to-end simulation frame, and assess the overall performance of the detector.Within ESAF, angular reconstruction can be separated into two conceptually different steps. The first step is pattern recognition, or filtering, of the signal to separate it from the background. The second step is to perform different types of fitting in order to search for the relevant geometrical parameters that best describe the previously selected signal. In this paper, we discuss some of the techniques we haveimplemented in ESAF to perform the geometrical reconstruction of EAS seen by JEM-EUSO. We also conduct thorough tests to assess the performances of these techniques in conditions which are relevant to the scope of the JEM-EUSO mission. We conclude by showing the expected angular resolution in the energy range that JEM-EUSO is expected to observe.
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, S.. Ecole Polytechnique; Francia
Fil: Albert, J. N.. Univ Paris-Sud; Francia
Fil: Allard, D.. Univ Paris Diderot; Francia
Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
Fil: Andreev, V.. University of California; Estados Unidos
Fil: Anzalone, A.. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Arai, Y.. High Energy Accelerator Research Organization; Japón
Fil: Asano, K.. Tokyo Institute of Technology; Japón
Fil: Ave Pernas, M.. Universidad de Alcala (UAH); España
Fil: Barrillon, P.. Univ Paris-Sud; Francia
Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
Fil: Bayer, J.. University of Tübingen; Alemania
Fil: Bechini, R.. Universita’ di Torino; Italia
Fil: Belenguer, T.. Instituto Nacional de Técnica Aeroespacial ; España
Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belov, K.. University of California; Estados Unidos
Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Biermann, P. L.. Karlsruhe Institute of Technology; Alemania
Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
Fil: Blaksley, C.. Univ Paris Diderot; Francia
Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology; Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences; Polonia
Fil: Blin-bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology; Alemania
Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia
Fil: Bogomilov, M.. University of Sofia; Bulgaria
Fil: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Guzman, A.. Institut f ur Astronomie und Astrophysik Tübingen; Alemania
Fil: Mernik, T.. Institut fur Astronomie und Astrophysik Tübingen; Alemania
Fil: The JEM-EUSO Collaboration.
Materia
Jem-Euso
Angular Reconstruction
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/18077

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network_name_str CONICET Digital (CONICET)
spelling Performances of JEM-EUSO: angular reconstruction The JEM-EUSO CollaborationAdams, J. H.Ahmad, S.Albert, J. N.Allard, D.Anchordoqui, L.Andreev, V.Anzalone, A.Arai, Y.Asano, K.Ave Pernas, M.Barrillon, P.Batsch, T.Bayer, J.Bechini, R.Belenguer, T.Bellotti, R.Belov, K.Berlind, A. A.Bertaina, M.Biermann, P. L.Biktemerova, S.Blaksley, C.Blanc, N.Blecki, J.Blin-bondil, S.Blumer, J.Bobik, P.Bogomilov, M.Bonamente, M.Supanitsky, Alberto DanielGuzman, A.Mernik, T.The JEM-EUSO CollaborationJem-EusoAngular Reconstructionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Mounted on the International Space Station(ISS), the Extreme UniverseSpace Observatory, on-board the Japanese Experimental Module (JEM-EUSO),relies on the well established fluorescence technique to observe Extensive Air Showers (EAS) developing in the earth?s atmosphere. Focusing on the detection of Ultra High Energy Cosmic Rays (UHECR) in the decade of 10 20 eV, JEM-EUSO will face new challenges by applying this technique from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed in this context to provide a full end-to-end simulation frame, and assess the overall performance of the detector.Within ESAF, angular reconstruction can be separated into two conceptually different steps. The first step is pattern recognition, or filtering, of the signal to separate it from the background. The second step is to perform different types of fitting in order to search for the relevant geometrical parameters that best describe the previously selected signal. In this paper, we discuss some of the techniques we haveimplemented in ESAF to perform the geometrical reconstruction of EAS seen by JEM-EUSO. We also conduct thorough tests to assess the performances of these techniques in conditions which are relevant to the scope of the JEM-EUSO mission. We conclude by showing the expected angular resolution in the energy range that JEM-EUSO is expected to observe.Fil: Adams, J. H.. University of Alabama in Huntsville; Estados UnidosFil: Ahmad, S.. Ecole Polytechnique; FranciaFil: Albert, J. N.. Univ Paris-Sud; FranciaFil: Allard, D.. Univ Paris Diderot; FranciaFil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados UnidosFil: Andreev, V.. University of California; Estados UnidosFil: Anzalone, A.. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; ItaliaFil: Arai, Y.. High Energy Accelerator Research Organization; JapónFil: Asano, K.. Tokyo Institute of Technology; JapónFil: Ave Pernas, M.. Universidad de Alcala (UAH); EspañaFil: Barrillon, P.. Univ Paris-Sud; FranciaFil: Batsch, T.. National Centre for Nuclear Research; PoloniaFil: Bayer, J.. University of Tübingen; AlemaniaFil: Bechini, R.. Universita’ di Torino; ItaliaFil: Belenguer, T.. Instituto Nacional de Técnica Aeroespacial ; EspañaFil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Belov, K.. University of California; Estados UnidosFil: Berlind, A. A.. Vanderbilt University; Estados UnidosFil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Biermann, P. L.. Karlsruhe Institute of Technology; AlemaniaFil: Biktemerova, S.. Joint Institute for Nuclear Research; RusiaFil: Blaksley, C.. Univ Paris Diderot; FranciaFil: Blanc, N.. Swiss Center for Electronics and Microtechnology; SuizaFil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences; PoloniaFil: Blin-bondil, S.. Ecole Polytechnique; FranciaFil: Blumer, J.. Karlsruhe Institute of Technology; AlemaniaFil: Bobik, P.. Institute of Experimental Physics; EslovaquiaFil: Bogomilov, M.. University of Sofia; BulgariaFil: Bonamente, M.. University of Alabama in Huntsville; Estados UnidosFil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Guzman, A.. Institut f ur Astronomie und Astrophysik Tübingen; AlemaniaFil: Mernik, T.. Institut fur Astronomie und Astrophysik Tübingen; AlemaniaFil: The JEM-EUSO Collaboration.Springer2015-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18077Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration; Springer; Experimental Astronomy; 40; 1; 11-2015; 153-1770922-6435enginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-013-9371-0info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-013-9371-0info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:56:20Zoai:ri.conicet.gov.ar:11336/18077instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:56:20.776CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
title Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
spellingShingle Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
Adams, J. H.
Jem-Euso
Angular Reconstruction
title_short Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
title_full Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
title_fullStr Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
title_full_unstemmed Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
title_sort Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration
dc.creator.none.fl_str_mv Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-bondil, S.
Blumer, J.
Bobik, P.
Bogomilov, M.
Bonamente, M.
Supanitsky, Alberto Daniel
Guzman, A.
Mernik, T.
The JEM-EUSO Collaboration
author Adams, J. H.
author_facet Adams, J. H.
Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-bondil, S.
Blumer, J.
Bobik, P.
Bogomilov, M.
Bonamente, M.
Supanitsky, Alberto Daniel
Guzman, A.
Mernik, T.
The JEM-EUSO Collaboration
author_role author
author2 Ahmad, S.
Albert, J. N.
Allard, D.
Anchordoqui, L.
Andreev, V.
Anzalone, A.
Arai, Y.
Asano, K.
Ave Pernas, M.
Barrillon, P.
Batsch, T.
Bayer, J.
Bechini, R.
Belenguer, T.
Bellotti, R.
Belov, K.
Berlind, A. A.
Bertaina, M.
Biermann, P. L.
Biktemerova, S.
Blaksley, C.
Blanc, N.
Blecki, J.
Blin-bondil, S.
Blumer, J.
Bobik, P.
Bogomilov, M.
Bonamente, M.
Supanitsky, Alberto Daniel
Guzman, A.
Mernik, T.
The JEM-EUSO Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Jem-Euso
Angular Reconstruction
topic Jem-Euso
Angular Reconstruction
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Mounted on the International Space Station(ISS), the Extreme UniverseSpace Observatory, on-board the Japanese Experimental Module (JEM-EUSO),relies on the well established fluorescence technique to observe Extensive Air Showers (EAS) developing in the earth?s atmosphere. Focusing on the detection of Ultra High Energy Cosmic Rays (UHECR) in the decade of 10 20 eV, JEM-EUSO will face new challenges by applying this technique from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed in this context to provide a full end-to-end simulation frame, and assess the overall performance of the detector.Within ESAF, angular reconstruction can be separated into two conceptually different steps. The first step is pattern recognition, or filtering, of the signal to separate it from the background. The second step is to perform different types of fitting in order to search for the relevant geometrical parameters that best describe the previously selected signal. In this paper, we discuss some of the techniques we haveimplemented in ESAF to perform the geometrical reconstruction of EAS seen by JEM-EUSO. We also conduct thorough tests to assess the performances of these techniques in conditions which are relevant to the scope of the JEM-EUSO mission. We conclude by showing the expected angular resolution in the energy range that JEM-EUSO is expected to observe.
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos
Fil: Ahmad, S.. Ecole Polytechnique; Francia
Fil: Albert, J. N.. Univ Paris-Sud; Francia
Fil: Allard, D.. Univ Paris Diderot; Francia
Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos
Fil: Andreev, V.. University of California; Estados Unidos
Fil: Anzalone, A.. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Arai, Y.. High Energy Accelerator Research Organization; Japón
Fil: Asano, K.. Tokyo Institute of Technology; Japón
Fil: Ave Pernas, M.. Universidad de Alcala (UAH); España
Fil: Barrillon, P.. Univ Paris-Sud; Francia
Fil: Batsch, T.. National Centre for Nuclear Research; Polonia
Fil: Bayer, J.. University of Tübingen; Alemania
Fil: Bechini, R.. Universita’ di Torino; Italia
Fil: Belenguer, T.. Instituto Nacional de Técnica Aeroespacial ; España
Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Belov, K.. University of California; Estados Unidos
Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos
Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Biermann, P. L.. Karlsruhe Institute of Technology; Alemania
Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia
Fil: Blaksley, C.. Univ Paris Diderot; Francia
Fil: Blanc, N.. Swiss Center for Electronics and Microtechnology; Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences; Polonia
Fil: Blin-bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology; Alemania
Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia
Fil: Bogomilov, M.. University of Sofia; Bulgaria
Fil: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Guzman, A.. Institut f ur Astronomie und Astrophysik Tübingen; Alemania
Fil: Mernik, T.. Institut fur Astronomie und Astrophysik Tübingen; Alemania
Fil: The JEM-EUSO Collaboration.
description Mounted on the International Space Station(ISS), the Extreme UniverseSpace Observatory, on-board the Japanese Experimental Module (JEM-EUSO),relies on the well established fluorescence technique to observe Extensive Air Showers (EAS) developing in the earth?s atmosphere. Focusing on the detection of Ultra High Energy Cosmic Rays (UHECR) in the decade of 10 20 eV, JEM-EUSO will face new challenges by applying this technique from space. The EUSO Simulation and Analysis Framework (ESAF) has been developed in this context to provide a full end-to-end simulation frame, and assess the overall performance of the detector.Within ESAF, angular reconstruction can be separated into two conceptually different steps. The first step is pattern recognition, or filtering, of the signal to separate it from the background. The second step is to perform different types of fitting in order to search for the relevant geometrical parameters that best describe the previously selected signal. In this paper, we discuss some of the techniques we haveimplemented in ESAF to perform the geometrical reconstruction of EAS seen by JEM-EUSO. We also conduct thorough tests to assess the performances of these techniques in conditions which are relevant to the scope of the JEM-EUSO mission. We conclude by showing the expected angular resolution in the energy range that JEM-EUSO is expected to observe.
publishDate 2015
dc.date.none.fl_str_mv 2015-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/18077
Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration; Springer; Experimental Astronomy; 40; 1; 11-2015; 153-177
0922-6435
url http://hdl.handle.net/11336/18077
identifier_str_mv Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Performances of JEM-EUSO: angular reconstruction The JEM-EUSO Collaboration; Springer; Experimental Astronomy; 40; 1; 11-2015; 153-177
0922-6435
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-013-9371-0
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-013-9371-0
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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