{"paper":{"title":"Search for Low-Mass Dark Matter with CDMSlite Using a Profile Likelihood Fit","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.CO","authors_text":"A.E. Robinson, A. Jastram, A. Kennedy, A. Kubik, A.N. Villano, A. Reisetter, A. Roberts, A. Scarff, B.A. Young, B. Cabrera, B. Cornell, B. Loer, B. Mohanty, B. Sadoulet, B. Serfass, B. von Krosigk, C. Cartaro, C. Jena, C. Stanford, C.W. Fink, D.A. Bauer, D. Barker, D.G. Cerde\\~no, D.H. Wright, D. Jardin, D. MacDonell, D. Speller, D. Toback, E. Azadbakht, E. Fascione, E. Figueroa-Feliciano, E. Lopez Asamar, E. Miller, E.W. Hoppe, F. De Brienne, F. Ponce, G. Gerbier, H.A. Tanaka, H.E. Rogers, H. Neog, H. Qiu, H.R. Harris, I.J. Arnquist, J. Cooley, J.D. Morales Mendoza, J.L. Orrell, J. Nelson, J. Sander, J. Street, J.S. Wilson, J. Winchell, K. Senapati, L. Hsu, M.A. Bowles, M.E. Huber, M. Fritts, M. Ghaith, M.H. Kelsey, M.J. Wilson, M. Pepin, M. Pyle, M. Stein, N.A. Kurinsky, N. Herbert, N. Mast, N. Mirabolfathi, P. Cushman, P.L. Brink, P. Lukens, R.A. Cameron, R. Bunker, R. Calkins, R.E. Lawrence, R. Germond, R. Mahapatra, R. Partridge, R. Ren, R. Underwood, R.W. Schnee, S. Banik, S.L. Watkins, S.M. Oser, S. Poudel, S.R. Golwala, S. Scorza, SuperCDMS Collaboration: R. Agnese, S. Yellin, T. Aralis, T. Aramaki, T. Binder, T. Doughty, T. Reynolds, T. Saab, V. Iyer, V. Mandic, W.A. Page, W. Baker, W. Rau, X. Zhang, X. Zhao, Y.-Y. Chang, Z. Hong","submitted_at":"2018-08-28T03:15:15Z","abstract_excerpt":"The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) searches for interactions between dark matter particles and germanium nuclei in cryogenic detectors. The experiment has achieved a low energy threshold with improved sensitivity to low-mass (<10 GeV/c$^2$) dark matter particles. We present an analysis of the final CDMSlite data set, taken with a different detector than was used for the two previous CDMSlite data sets. This analysis includes a data \"salting\" method to protect against bias, improved noise discrimination, background modeling, and the use of profile li"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.09098","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1808.09098/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}