{"paper":{"title":"Low Energy Analysis Techniques for CUORE","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"physics.ins-det","authors_text":"A. Bersani, A. Branca, A. Camacho, A. Caminata, A. D'Addabbo, A. Drobizhev, A. Giachero, A. Giuliani, A. Leder, A. Nucciotti, A. R. Smith, A. Woodcraft, B. K. Fujikawa, B. Schmidt, B. S. Wang, B. Welliver, C. Brofferio, C. Bucci, C. Cosmelli, C. E. Pagliarone, C. Gotti, C. J. Davis, C. Ligi, C. Nones, C. Pira, C. Rosenfeld, C. Rusconi, C. Tomei, CUORE Collaboration: C. Alduino, D. Chiesa, D. D'Aguanno, D. Q. Fang, D. R. Artusa, D. Santone, E. B. Norman, E. E. Haller, E. Ferri, E. Fiorini, E. Hansen, E. Previtali, F. Bellini, F. Ferroni, F. T. Avignone III, F. Terranova, G. Bari, G. Benato, G. Keppel, G. Pessina, G. Piperno, G. Q. Zhang, H. W. Wang, H. Z. Huang, I. Dafinei, J. L. Ouellet, J. Schmidt, J. S. Cushman, J.W. Beeman, J. Wilson, K. Alfonso, K. E. Lim, K. Han, K. M. Heeger, L. A. Winslow, L. Canonica, L. Cappelli, L. Cardani, L. Cassina, L. Gironi, L. Gladstone, L. Marini, L. Pattavina, L. Taffarello, L. Zanotti, M. A. Franceschi, M. Biassoni, M. Clemenza, M. Faverzani, M. L. di Vacri, M. Maino, M. Martinez, M. M. Deninno, M. Nastasi, M. Pallavicini, M. Pavan, M. Sakai, M. Sisti, M. Vignati, N. Casali, N. Chott, N. D. Scielzo, N. Moggi, O. Azzolini, O. Cremonesi, P. Carniti, P. Gorla, P. J. Mosteiro, R. Hennings-Yeomans, R. H. Maruyama, R. J. Creswick, R. Kadel, S. Capelli, S. Copello, S. Dell'Oro, S. Di Domizio, S. J. Freedman, S. L. Wagaarachchi, S. Morganti, S. Pirro, S. Pozzi, S. Sangiorgio, S. Zimmermann, S. Zucchelli, T. D. Gutierrez, T. Napolitano, T. O'Donnell, T. Wise, V. Novati, V. Palmieri, V. Singh, X. G. Cao, Y. G. Ma, Y. Mei, Yu. G. Kolomensky","submitted_at":"2017-08-25T17:03:06Z","abstract_excerpt":"CUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of $^{130}$Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searches requires improving the energy threshold to 10 keV. In this paper, we describe the analysis techniques developed for the low energy analysis of CUORE-like detectors, using the data acquired from No"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.07809","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}