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Comparison of available measurements of the absolute air-fluorescence yield and determination of its global average value

dc.book.titleInternational Symposium on the Recent Progress of Ultra-High Energy Cosmic Ray Observation
dc.contributor.authorRosado Vélez, Jaime
dc.contributor.authorBlanco Ramos, Francisco
dc.contributor.authorArqueros Martínez, Fernando
dc.date.accessioned2023-06-20T05:48:04Z
dc.date.available2023-06-20T05:48:04Z
dc.date.issued2011
dc.description© 2011 American Institute of Physics. ISSN: 0094-243X International Symposium on the Recent Progress of Ultra-High Energy Cosmic Ray Observation (2010. Aichi, Japón) This work has been supported by the Spanish Ministerio de Ciencia e Innovacion (FPA2009-07772 and CONSOLIDER CPAN CSD2007-42) and “Comunidad de Madrid” (Ref.: 910600). J. Rosado acknowledges a PhD grant from “Universidad Complutense de Madrid”. The authors thank our colleagues of the Auger collaboration for fruitful discussions and comments on this work.
dc.description.abstractExperimental results of the absolute air-fluorescence yield are given very often in different units (photons/MeV or photons/m) and for different wavelength intervals. In this work we present a comparison of available results normalized to its value in photons/MeV for the 337 nm band at 1013 hPa and 293 K. The conversion of photons/m to photons/MeV requires an accurate determination of the energy deposited by the electrons in the field of view of the experimental set-up. We have calculated the energy deposition for each experiment by means of a detailed Monte Carlo simulation and the results have been compared with those assumed or calculated by the authors. As a result, corrections to the reported fluorescence yields are proposed. These corrections improve the compatibility between measurements in such a way that a reliable average value with uncertainty at the level of 5% is obtained.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)
dc.description.sponsorshipComunidad de Madrid
dc.description.sponsorshipUniversidad Complutense de Madrid
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/38587
dc.identifier.doi10.1063/1.3628711
dc.identifier.isbn978-0-7354-0927-9
dc.identifier.officialurlhttp://dx.doi.org/10.1063/1.3628711
dc.identifier.relatedurlhttp://scitation.aip.org/
dc.identifier.relatedurlhttp://arxiv.org/abs/1104.0894
dc.identifier.urihttps://hdl.handle.net/20.500.14352/45645
dc.language.isoeng
dc.page.final39
dc.page.initial34
dc.page.total34
dc.publisherAmerican Institute of Physics
dc.relation.ispartofseriesAIP Conference Proceedings
dc.relation.projectIDFPA2009-07772
dc.relation.projectIDCONSOLIDER CPAN CSD2007-42
dc.relation.projectID910600
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordElectron beam
dc.subject.keywordPhoton yields
dc.subject.keywordNitrogen
dc.subject.keywordEmission
dc.subject.keywordNM
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleComparison of available measurements of the absolute air-fluorescence yield and determination of its global average value
dc.typebook part
dc.volume.number1367
dcterms.references[1] F. Kakimoto et al., Nucl. Instr. and Meth. A 372 527 (1996). [2] M. Nagano et al., Astropart. Phys. 22 235 (2004). [3] G. Lefeuvre et al., Nucl. Instr. and Meth. A 578 78 (2007). [4] P. Colin et al. [MACFLY Collaboration], Astropart. Phys. 27 317 (2007). [5] T. Waldenmaier et al., Astropart. Phys. 29 205 (2008). [6] R. Abbasi et al. [FLASH Collaboration], Astropart. Phys. 29 77 (2008). [7] P. Privitera, Proceedings of this conference. [8] F. Blanco and F. Arqueros, Phys. Lett A 345 355 (2005). [9] F. Arqueros et al., Astropart. Phys. 26 231 (2006). [10] F. Arqueros et al., New J. Phys. 11 065011 (2009). [11] M. Ave et al. [AIRFLY Collaboration], Astropart. Phys. 28 41 (2007). [12] The AIRFLY Collaboration, private communication. [13] J. Rosado et al., Astropart. Phys. 34 164 (2010). [14] M. Nagano et al., Astropart. Phys. 20 293 (2003). [15] In this section we show preliminary results of a work in preparation (available in arXiv:1103.2022) [16] F. Arqueros et al., Proceedings of 43rd Rencontres de Moriond – Electroweak Interactions and Unified Theories (La Thuile, Italy, 2008). Available in arXiv:0807.4824
dspace.entity.typePublication
relation.isAuthorOfPublication32033072-414c-4448-b44b-98a6bd3e9321
relation.isAuthorOfPublicationfd97b031-5b10-40ab-beb5-8f192e632ca3
relation.isAuthorOfPublicatione6fd6d50-2946-45a9-a515-273dddff2091
relation.isAuthorOfPublication.latestForDiscovery32033072-414c-4448-b44b-98a6bd3e9321

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