{"paper":{"title":"QUBIC III: Laboratory Characterization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Almela, A. Ba\\`u, A.C. Cobos Cerutti, A. Coppolecchia, A.D. Supanitsky, A. Etchegoyen, A. Fasciszewski, 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, C. Chapron, C. Duca, 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. Melo, D. Pr\\^ele, D. Rambaud, D. Vigan\\`o, E. Bunn, E. Jules, E. Olivieri, E. Rasztocky, E.S. Battistelli, F. Cavaliere, F. Columbro, F. Incardona, F. Nati, F. Pajot, F. Pezzotta, F. Piacentini, F. Voisin, F. Wicek, G. Amico, 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.M. 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. 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.R. Hampel, M. Stolpovskiy, M. Tomasi, M. Wright, M. Zannoni, N. Vittorio, P. Ade, P. Chanial, P. De Bernardis, P. Ringegni, P. Timbie, R. Charlassier, R. Puddu, S.A. Torchinsky, S. Azzoni, S. Banfi, S. Dheilly, S. Henrot-Versill\\'e, S. Loucatos, S. Marnieros, S. Masi, S. Scully, S. Spinelli, T. Louis, V. Gilles, W. Marty, Y. Giraud-Heraud","submitted_at":"2020-08-23T15:09:42Z","abstract_excerpt":"A prototype version of the Q & U Bolometric Interferometer for Cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology in Paris. We report the results of this Technological Demonstrator which successfully shows the feasibility of the principle of Bolometric Interferometry. Characterization of QUBIC includes the measurement of the synthesized beam, the measurement of interference fringes, and the measurement of polarization performance. A modulated and frequency tunable millimetre-wave source in the telescope far-field is used to simulate a poi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.10056","kind":"arxiv","version":4},"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/2008.10056/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"}