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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18077
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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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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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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13.070432 |