PoS - Proceedings of Science
Volume 441 - XVIII International Conference on Topics in Astroparticle and Underground Physics (TAUP2023) - Dark Matter and its Detection
Confirmation of the excess of ionization events in DAMIC at SNOLAB with skipper CCDs
M. Traina*,  DAMIC, DAMIC-M and SENSEI, A. Aguilar-Arevalo, I. Arnquist, N. Avalos, L. Barak, D. Baxter, X. Bertou, I.M. Bloch, A.M. Botti, M. Cababie, G. Cancelo, N. Castello-Mor, B.A. Cervantes-Vergara, A.E. Chavarria, J. Cortabitarte-Gutiérrez, M. Crisler, J. Cuevas-Zepeda, A. Dastgheibi-Fard, C. De Dominicis, O. Deligny, A. Drlica-Wagner, J. Duarte-Campderros, J.C. D'Olivo, R. Essig, E. Estrada, J. Estrada, E. Etzion, F. Favela-Perez, N. Gadola, R. Gaior, S.E. Holland, T. Hossbach, L. Iddir, B. Kilminster, Y. Korn, A. Lantero-Barreda, I.T. Lawson, S.C. Lee, A. Letessier-Selvon, P. Loaiza, A. Lopez-Virto, S. Luoma, E. Marrufo-Villalpando, K.J. McGuire, G.F. Moroni, S. Munagavalasa, D. Norcini, A. Orly, G. Papadopoulos, S. Paul, S.E. Perez, A. Piers, P. Privitera, P. Robmann, D. Rodrigues, N.A. Saffold, S. Scorza, M. Settimo, A. Singal, R. Smida, M. Sofo-Haro, L. Stefanazzi, K. Stifter, J. Tiffenberg, M. Traina, S. Uemura, I. Vila, R. Vilar, T. Volansky, G. Warot, R. Yajur, T.T. Yu and J.P. Zopounidiset al. (click to show)
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Pre-published on: February 20, 2024
Published on: March 22, 2024
Abstract
We present results from a 3.2 kg-day target exposure of two 24-megapixel skipper charge-coupled devices (CCDs) deployed in the DAMIC setup at SNOLAB. With a $10\times$ reduction in pixel noise, we investigate the excess population of low-energy bulk events 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 observed energy spectrum and spatial distribution of ionization events with electron-equivalent energies ${<}500$ eV confirm the presence of a bulk excess compatible with previous findings. This measurement establishes the existence of a prominent source of low-energy events in the CCD target with characteristic rate of ${\sim}7$ events per kg-day, and energies ${\sim}80$ eV, whose origin remains unknown.
DOI: https://doi.org/10.22323/1.441.0059
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