Calibration aspects of the JEM-EUSO mission
- 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; The JEM-EUSO Collaboration
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper.
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 (KEK); 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 Tubingen; Alemania
Fil: Bechini, R.. Universita’ di Torino; Italia
Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); 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 (KIT); 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 (CSEM); Suiza
Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia
Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia
Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); 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: The JEM-EUSO Collaboration. - Materia
-
Air-Shower Fluorescence Telescope
Jem-Euso
Calibration
Space-Based Experiment - 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:11336/17897
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Calibration aspects of the JEM-EUSO missionAdams, 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 DanielThe JEM-EUSO CollaborationAir-Shower Fluorescence TelescopeJem-EusoCalibrationSpace-Based Experimenthttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper.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 (KEK); 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 Tubingen; AlemaniaFil: Bechini, R.. Universita’ di Torino; ItaliaFil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); 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 (KIT); AlemaniaFil: Biktemerova, S.. Joint Institute for Nuclear Research; RusiaFil: Blaksley, C.. Univ Paris Diderot; FranciaFil: Blanc. N.. Swiss Center for Electronics and Microtechnology (CSEM); SuizaFil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); PoloniaFil: Blin-Bondil, S.. Ecole Polytechnique; FranciaFil: Blumer, J.. Karlsruhe Institute of Technology (KIT); 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: 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/11336/17897Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Calibration aspects of the JEM-EUSO mission; Springer; Experimental Astronomy; 40; 1; 11-2015; 91-1160922-6435enginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10686-015-9453-2info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-015-9453-2info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:32:27Zoai:ri.conicet.gov.ar:11336/17897instacron: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 09:32:27.567CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Calibration aspects of the JEM-EUSO mission |
title |
Calibration aspects of the JEM-EUSO mission |
spellingShingle |
Calibration aspects of the JEM-EUSO mission Adams, J. H. Air-Shower Fluorescence Telescope Jem-Euso Calibration Space-Based Experiment |
title_short |
Calibration aspects of the JEM-EUSO mission |
title_full |
Calibration aspects of the JEM-EUSO mission |
title_fullStr |
Calibration aspects of the JEM-EUSO mission |
title_full_unstemmed |
Calibration aspects of the JEM-EUSO mission |
title_sort |
Calibration aspects of the JEM-EUSO mission |
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 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 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 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 |
dc.subject.none.fl_str_mv |
Air-Shower Fluorescence Telescope Jem-Euso Calibration Space-Based Experiment |
topic |
Air-Shower Fluorescence Telescope Jem-Euso Calibration Space-Based Experiment |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper. 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 (KEK); 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 Tubingen; Alemania Fil: Bechini, R.. Universita’ di Torino; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); 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 (KIT); 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 (CSEM); Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); 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: The JEM-EUSO Collaboration. |
description |
he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper. |
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/11336/17897 Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Calibration aspects of the JEM-EUSO mission; Springer; Experimental Astronomy; 40; 1; 11-2015; 91-116 0922-6435 |
url |
http://hdl.handle.net/11336/17897 |
identifier_str_mv |
Adams, J. H.; Ahmad, S.; Albert, J. N.; Allard, D.; Anchordoqui, L.; et al.; Calibration aspects of the JEM-EUSO mission; Springer; Experimental Astronomy; 40; 1; 11-2015; 91-116 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/s10686-015-9453-2 info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-015-9453-2 |
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 |
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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 |