dc.contributor.author | Aguilar Arévalo, A. | |
dc.contributor.author | Castelló Mor, Nuria | |
dc.contributor.author | Cortabitarte Gutiérrez, Juan | |
dc.contributor.author | Duarte Campderros, Jorge | |
dc.contributor.author | Lantero Barreda, Agustín | |
dc.contributor.author | López Virto, María Amparo | |
dc.contributor.author | Vila Álvarez, Iván | |
dc.contributor.author | Vilar Cortabitarte, Rocío | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2024-05-23T14:41:08Z | |
dc.date.available | 2024-05-23T14:41:08Z | |
dc.date.issued | 2024-03 | |
dc.identifier.issn | 1550-7998 | |
dc.identifier.issn | 1550-2368 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.issn | 2470-0029 | |
dc.identifier.other | PID2019-109829 GB-I00 | es_ES |
dc.identifier.uri | https://hdl.handle.net/10902/32911 | |
dc.description.abstract | We 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.sponsorship | We 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.extent | 8 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | American Physical Society | es_ES |
dc.rights | © 2024 American Physical Society | es_ES |
dc.source | Physical Review D, 2024, 109(6), 062007 | es_ES |
dc.title | Confirmation of the spectral excess in DAMIC at SNOLAB with skipper CCDs | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1103/PhysRevD.109.062007 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1103/PhysRevD.109.062007 | |
dc.type.version | publishedVersion | es_ES |