<?xml version="1.0" encoding="UTF-8"?>
<collection>
<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1007/JHEP10(2019)230</dc:identifier><dc:language>eng</dc:language><dc:creator>Renner, J.</dc:creator><dc:creator>Díaz López, G.</dc:creator><dc:creator>Ferrario, P.</dc:creator><dc:creator>Hernando Morata, J.A.</dc:creator><dc:creator>Kekic, M.</dc:creator><dc:creator>Martínez-Lema, G.</dc:creator><dc:creator>Monrabal, F.</dc:creator><dc:creator>Gómez-Cadenas, J.J.</dc:creator><dc:creator>Adams, C.</dc:creator><dc:creator>Álvarez, V.</dc:creator><dc:creator>Arazi, L.</dc:creator><dc:creator>Arnquist, I.J.</dc:creator><dc:creator>Azevedo, C.D.R.</dc:creator><dc:creator>Bailey, K.</dc:creator><dc:creator>Ballester, F.</dc:creator><dc:creator>Benlloch-Rodríguez, J.M.</dc:creator><dc:creator>Borges, F.I.G.M.</dc:creator><dc:creator>Byrnes, N.</dc:creator><dc:creator>Cárcel, S.</dc:creator><dc:creator>Carrión, J.V.</dc:creator><dc:creator>Cebrián, S.</dc:creator><dc:creator>Church, E.</dc:creator><dc:creator>Conde, C.A.N.</dc:creator><dc:creator>Contreras, T.</dc:creator><dc:creator>Díaz, J.</dc:creator><dc:creator>Diesburg, M.</dc:creator><dc:creator>Escada, J.</dc:creator><dc:creator>Esteve, R.</dc:creator><dc:creator>Felkai, R.</dc:creator><dc:creator>Fernandes, A.F.M.</dc:creator><dc:creator>Fernandes, L.M.P.</dc:creator><dc:creator>Ferreira, A.L.</dc:creator><dc:creator>Freitas, E.D.C.</dc:creator><dc:creator>Generowicz, J.</dc:creator><dc:creator>Ghosh, S.</dc:creator><dc:creator>Goldschmidt, A.</dc:creator><dc:creator>González-Díaz, D.</dc:creator><dc:creator>Guenette, R.</dc:creator><dc:creator>Gutiérrez, R.M.</dc:creator><dc:creator>Haefner, J.</dc:creator><dc:creator>Hafidi, K.</dc:creator><dc:creator>Hauptman, J.</dc:creator><dc:creator>Henriques, C.A.O.</dc:creator><dc:creator>Herrero, P.</dc:creator><dc:creator>Herrero, V.</dc:creator><dc:creator>Ifergan, Y.</dc:creator><dc:creator>Johnston, S.</dc:creator><dc:creator>Jones, B.J.P.</dc:creator><dc:creator>Labarga, L.</dc:creator><dc:creator>Laing, A.</dc:creator><dc:creator>Lebrun, P.</dc:creator><dc:creator>López-March, N.</dc:creator><dc:creator>Losada, M.</dc:creator><dc:creator>Mano, R.D.P.</dc:creator><dc:creator>Martín-Albo, J.</dc:creator><dc:creator>Martínez, A.</dc:creator><dc:creator>McDonald, A.D.</dc:creator><dc:creator>Monteiro, C.M.B.</dc:creator><dc:creator>Mora, F.J.</dc:creator><dc:creator>Muñoz Vidal, J.</dc:creator><dc:creator>Novella, P.</dc:creator><dc:creator>Nygren, D.R.</dc:creator><dc:creator>Palmeiro, B.</dc:creator><dc:creator>Para, A.</dc:creator><dc:creator>Pérez, J.</dc:creator><dc:creator>Psihas, F.</dc:creator><dc:creator>Querol, M.</dc:creator><dc:creator>Repond, J.</dc:creator><dc:creator>Riordan, S.</dc:creator><dc:creator>Ripoll, L.</dc:creator><dc:creator>Rodríguez García, Y.</dc:creator><dc:creator>Rodríguez, J.</dc:creator><dc:creator>Rogers, L.</dc:creator><dc:creator>Romeo, B.</dc:creator><dc:creator>Romo-Luque, C.</dc:creator><dc:creator>Santos, F.P.</dc:creator><dc:creator>dos Santos, J.M.F.</dc:creator><dc:creator>Simón, A.</dc:creator><dc:creator>Sofka, C.</dc:creator><dc:creator>Sorel, M.</dc:creator><dc:creator>Stiegler, T.</dc:creator><dc:creator>Toledo, J.F.</dc:creator><dc:creator>Torrent, J.</dc:creator><dc:creator>Usón, A.</dc:creator><dc:creator>Veloso, J.F.C.A.</dc:creator><dc:creator>Webb, R.</dc:creator><dc:creator>Weiss-Babai, R.</dc:creator><dc:creator>White, J.T.</dc:creator><dc:creator>Woodruff, K.</dc:creator><dc:creator>Yahlali, N.</dc:creator><dc:creator>The NEXT collaboration</dc:creator><dc:title>Energy calibration of the NEXT-White detector with 1% resolution near Qßß of 136Xe</dc:title><dc:identifier>ART-2019-114950</dc:identifier><dc:description>Excellent energy resolution is one of the primary advantages of electroluminescent high-pressure xenon TPCs. These detectors are promising tools in searching for rare physics events, such as neutrinoless double-beta decay (ßß0¿), which require precise energy measurements. Using the NEXT-White detector, developed by the NEXT (Neutrino Experiment with a Xenon TPC) collaboration, we show for the first time that an energy resolution of 1% FWHM can be achieved at 2.6 MeV, establishing the present technology as the one with the best energy resolution of all xenon detectors for ßß0¿ searches. [Figure not available: see fulltext.</dc:description><dc:date>2019</dc:date><dc:source>http://zaguan.unizar.es/record/86358</dc:source><dc:doi>10.1007/JHEP10(2019)230</dc:doi><dc:identifier>http://zaguan.unizar.es/record/86358</dc:identifier><dc:identifier>oai:zaguan.unizar.es:86358</dc:identifier><dc:relation>info:eu-repo/grantAgreement/EC/FP7/339787/EU/Towards the NEXT generation of bb0nu experimets/NEXT</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/RTI2018-095979</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/FIS2014-53371-C04</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/MDM-2016-0692</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/RYC-2015-18820</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/SEV-2014-0398</dc:relation><dc:identifier.citation>Journal of High Energy Physics 2019, 10 (2019), 230  1-11</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>http://creativecommons.org/licenses/by/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

</collection>