{"paper":{"title":"QUBIC: using NbSi TESs with a bolometric interferometer to characterize the polarisation of the CMB","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.IM","authors_text":"A. Almela, A. Ba\\`u, A. Bottani, A. Buzzelli, A. Coppolecchia, A. Di Donato, A. Etchegoyen, A. Fasciszewski, A. Gault, A. Korotkov, A. Mattei, A. May, A. Mennella, A. Paiella, A. Passerini, A. Pelosi, A. Schillaci, A. Tartari, A. Zullo, B. B\\'elier, B. Garc\\'ia, B. Maffei, B. Watson, C. Chapron, C. Franceschet, C. Kristukat, C. Oriol, C. O'Sullivan, C. Perbost, C. Sc\\'occola, C. Tucker, D. Auguste, D. Bennett, D. Burke, D. Buzi, D. Fracchia, D. Gayer, D. Harari, D. Pr\\^ele, D. Rambaud, D.T. Hoang, D. Vigan\\`o, E. Bunn, E. Jules, E. Olivieri, E.S. Battistelli, F. Cavaliere, F. Columbro, F. Incardona, F. Nati, F. Pajot, F. Pezzotta, F. Piacentini, F. Suarez, F. Voisin, F. Wicek, G. Amico, G. Coppi, G. D'Alessandro, G. De Gasperis, G. E. Romero, G. Pisano, G. Polenta, G. Stankowiak, G. Tucker, H. Pastoriza, J. A. Murphy, J. Aumont, J. Bonaparte, J. Bonis, J.-Ch. Hamilton, J.D. Murphy, J.G. Alberro, J. Kaplan, J.M. Salum, J.-Ph. Bernard, J.-P. Thermeau, K. Ganga, L. Berg\\'e, L. Dumoulin, L. Grandsire, L. H. Arnaldi, L. Lamagna, L. Mele, L. M. Mundo, L. Montier, L. Mousset, L.P. Ferreyro, L. Piccirillo, M.-A. Bigot-Sazy, M. Bersanelli, M.C. Medina, M. De Leo, M. De Petris, M.E. Garc\\'ia Redondo, M. Gaspard, M. Gervasi, M. Giard, M. G\\'omez Berisso, M. Gonz\\'alez, M. Gradziel, M. McCulloch, M.M. Gamboa Lerena, M. Perciballi, M. Piat, M. Platino, M. Salatino, M. Stolpovskiy, M. Tomasi, M. Zannoni, N. Bleurvacq, N. Vittorio, P. Ade, P. Battaglia, P. Chanial, P. De Bernardis, P. Ringegni, P. Timbie, R. Charlassier, R. Luterstein, R. Puddu, S. Azzoni, S. Banfi, S. Dheilly, S. Henrot-Versill\\'e, S. Loucatos, S. Marnieros, S. Masi, S. Melhuish, S. Scully, S. Spinelli, S. Torchinsky, S. Vanneste, T. Louis, V. Gilles, V. Haynes, W. Marty, Y. Giraud-Heraud","submitted_at":"2019-11-27T20:49:23Z","abstract_excerpt":"QUBIC (Q \\& U Bolometric Interferometer for Cosmology) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background (CMB). It is based on bolometric interferometry, an original detection technique which combine the immunity to systematic effects of an interferometer with the sensitivity of low temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta province.\n  The QUBIC detection chain consists in 2048 NbSi Transition Edge"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1911.12418","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1911.12418/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"}