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dc.contributor.author
Adams, J. H.  
dc.contributor.author
Ahmad, S.  
dc.contributor.author
Albert, J. N.  
dc.contributor.author
Allard, D.  
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Anchordoqui, L.  
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Andreev, V.  
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Anzalone, A.  
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Arai, Y.  
dc.contributor.author
Asano, K.  
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Ave Pernas, M.  
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Barrillon, P.  
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Batsch, T.  
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Bayer, J.  
dc.contributor.author
Bechini, R.  
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Belenguer, T.  
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Bellotti, R.  
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Belov, K.  
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Berlind, A. A.  
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Bertaina, M.  
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Biermann, P. L.  
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Biktemerova, S.  
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Blaksley, C.  
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Blanc. N.  
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Blecki, J.  
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Blin-Bondil, S.  
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Blumer, J.  
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Bobik, P.  
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Bogomilov, M.  
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Bonamente, M.  
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Supanitsky, Alberto Daniel  
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The JEM-EUSO Collaboration  
dc.date.available
2017-06-09T19:00:22Z  
dc.date.issued
2015-11  
dc.identifier.citation
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  
dc.identifier.issn
0922-6435  
dc.identifier.uri
http://hdl.handle.net/11336/17897  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Springer  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Air-Shower Fluorescence Telescope  
dc.subject
Jem-Euso  
dc.subject
Calibration  
dc.subject
Space-Based Experiment  
dc.subject.classification
Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Calibration aspects of the JEM-EUSO mission  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2017-06-06T14:49:40Z  
dc.journal.volume
40  
dc.journal.number
1  
dc.journal.pagination
91-116  
dc.journal.pais
Alemania  
dc.journal.ciudad
Berlin  
dc.description.fil
Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos  
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Fil: Ahmad, S.. Ecole Polytechnique; Francia  
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Fil: Albert, J. N.. Univ Paris-Sud; Francia  
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Fil: Allard, D.. Univ Paris Diderot; Francia  
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Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos  
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Fil: Andreev, V.. University of California; Estados Unidos  
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Fil: Anzalone, A.. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia  
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Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón  
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Fil: Asano, K.. Tokyo Institute of Technology; Japón  
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Fil: Ave Pernas, M.. Universidad de Alcala (UAH); España  
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Fil: Barrillon, P.. Univ Paris-Sud; Francia  
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Fil: Batsch, T.. National Centre for Nuclear Research; Polonia  
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Fil: Bayer, J.. University of Tubingen; Alemania  
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Fil: Bechini, R.. Universita’ di Torino; Italia  
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Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España  
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Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia  
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Fil: Belov, K.. University of California; Estados Unidos  
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Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos  
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Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia  
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Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania  
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Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia  
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Fil: Blaksley, C.. Univ Paris Diderot; Francia  
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Fil: Blanc. N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza  
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Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia  
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Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia  
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Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania  
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Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia  
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Fil: Bogomilov, M.. University of Sofia; Bulgaria  
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Fil: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos  
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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  
dc.description.fil
Fil: The JEM-EUSO Collaboration.  
dc.journal.title
Experimental Astronomy  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/s10686-015-9453-2  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/s10686-015-9453-2