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   <dc:title>On the absolute value of the air-fluorescence yield</dc:title>
   <dc:creator>Rosado Vélez, Jaime</dc:creator>
   <dc:creator>Blanco Ramos, Francisco</dc:creator>
   <dc:creator>Arqueros Martínez, Fernando</dc:creator>
   <dc:subject>539.1</dc:subject>
   <dc:subject>Electron-impact</dc:subject>
   <dc:subject>Cross-sections</dc:subject>
   <dc:subject>Secondary electrons</dc:subject>
   <dc:subject>Cosmic-rays</dc:subject>
   <dc:subject>Nitrogen</dc:subject>
   <dc:subject>Pressure</dc:subject>
   <dc:subject>Detector</dc:subject>
   <dc:subject>State</dc:subject>
   <dc:subject>Beam</dc:subject>
   <dc:subject>NM</dc:subject>
   <dc:subject>Física nuclear</dc:subject>
   <dc:subject>2207 Física Atómica y Nuclear</dc:subject>
   <dc:description>© Elsevier Science BV 2014.
This work was supported by MINECO (FPA2009-07772, FPA2012-39489-C04-02) and CONSOLIDER CPAN CSD2007-42. We thank our colleagues of the Auger Collaboration for fruitful discussions and comments on this work.</dc:description>
   <dc:description>The absolute value of the air-fluorescence yield is a key parameter for the energy reconstruction of extensive air showers registered by fluorescence telescopes. In previous publications, we reported a detailed Monte Carlo simulation of the air-fluorescence generation that allowed the theoretical evaluation of this parameter. This simulation has been upgraded in the present work. As a result, we determined an updated absolute value of the fluorescence yield of 7.9 +/- 2.0 ph/MeV for the band at 337 nm in dry air at 800 hPa and 293 K, in agreement with experimental values. We have also performed a critical analysis of available absolute measurements of the fluorescence yield with the assistance of our simulation. Corrections have been applied to some measurements to account for a bias in the evaluation of the energy deposition. Possible effects of other experimental aspects have also been discussed. From this analysis, we determined an average fluorescence yield of 7.04 +/- 0.24 ph/MeV at the above conditions. (C) 2014 Elsevier B.V. All rights reserved.</dc:description>
   <dc:description>Ministerio de Economía y Competitividad (MINECO)</dc:description>
   <dc:description>CONSOLIDER CPAN</dc:description>
   <dc:description>Depto. de Estructura de la Materia, Física Térmica y Electrónica</dc:description>
   <dc:description>Fac. de Ciencias Físicas</dc:description>
   <dc:description>TRUE</dc:description>
   <dc:description>pub</dc:description>
   <dc:date>2023-06-19T14:55:32Z</dc:date>
   <dc:date>2023-06-19T14:55:32Z</dc:date>
   <dc:date>2014-03</dc:date>
   <dc:type>journal article</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/34804</dc:identifier>
   <dc:identifier>0927-6505</dc:identifier>
   <dc:identifier>10.1016/j.astropartphys.2014.02.003</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>FPA2009-07772</dc:relation>
   <dc:relation>FPA2012-39489-004-02</dc:relation>
   <dc:relation>CSD2007-42</dc:relation>
   <dc:rights>open access</dc:rights>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>Elsevier Science BV</dc:publisher>
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