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dc.contributor.authorAguilar Arévalo, A.
dc.contributor.authorCastelló Mor, Nuria 
dc.contributor.authorCortabitarte Gutiérrez, Juan
dc.contributor.authorDuarte Campderros, Jorge 
dc.contributor.authorLantero Barreda, Agustín
dc.contributor.authorLópez Virto, María Amparo
dc.contributor.authorVila Álvarez, Iván  
dc.contributor.authorVilar Cortabitarte, Rocío 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-05-23T14:41:08Z
dc.date.available2024-05-23T14:41:08Z
dc.date.issued2024-03
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.otherPID2019-109829 GB-I00es_ES
dc.identifier.urihttps://hdl.handle.net/10902/32911
dc.description.abstractWe present results from a 3.25 kg-day target exposure of two silicon charge-coupled devices (CCDs), each with 24 megapixels and skipper readout, deployed in the DAMIC setup at SNOLAB. With a reduction in pixel readout noise of a factor of 10 relative to the previous detector, we investigate the excess population of low-energy events in the CCD bulk previously observed above expected backgrounds. We address the dominant systematic uncertainty of the previous analysis through a depth fiducialization designed to reject surface backgrounds on the CCDs. The measured bulk ionization spectrum confirms the presence of an excess population of low-energy events in the CCD target with characteristic rate of ∼7 events per kg-day and electron-equivalent energies of ∼80 eV, whose origin remains unknown.es_ES
dc.description.sponsorshipWe acknowledge financial support from the following agencies and organizations: NSF through Grant No. NSF PHY-2110585 to the University of Washington and the University of Chicago; the Kavli Institute for Cosmological Physics at the University of Chicago through an endowment from the Kavli Foundation; the U.S. Department of Energy Office of Science through the Dark Matter New Initiatives program; Fermi National Accelerator Laboratory (Contract No. DEAC02-07CH11359); Institut Lagrange de Paris Laboratoire d’Excellence (under Reference No. ANR-10-LABX-63) supported by French state funds managed by the Agence Nationale de la Recherche within the Investissements d’Avenir program under Reference No. ANR-11-IDEX0004-02; Swiss National Science Foundation through Grant No. 200021_153654 and via the Swiss Canton of Zurich; IFCA through Project No. PID2019–109829 GB-I00 funded by MCIN/AEI; Mexico’s Consejo Nacional de Ciencia y Tecnología (Grant No. CF-2023-I-1169) and Dirección General de Asuntos del Personal Académico–Universidad Nacional Autónoma de México (Programa de Apoyo a Proyectos de Investigación e Innovación Tecnológica Grant No. IN106322).es_ES
dc.format.extent8 p.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rights© 2024 American Physical Societyes_ES
dc.sourcePhysical Review D, 2024, 109(6), 062007es_ES
dc.titleConfirmation of the spectral excess in DAMIC at SNOLAB with skipper CCDses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1103/PhysRevD.109.062007es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1103/PhysRevD.109.062007
dc.type.versionpublishedVersiones_ES


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