{"paper":{"title":"QUBIC IV: Performance of TES Bolometers and Readout Electronics","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Almela, A. Bau, 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. Belier, B. Garcia, B. Maffei, C. Chapron, C. Duca, C. Franceschet, C.G. Scoccola, C. Kristukat, C. Oriol, C. O Sullivan, C. Perbost, C. Tucker, D. Auguste, D. Bennett, D. Burke, D. Buzi, D. Fracchia, D. Gayer, D. Harari, D. Melo, D. Prele, D. Rambaud, D. Vigano, 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. Berge, 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. Garcia Redondo, M. Gaspard, M. Gervasi, M. Giard, M. Gomez Berisson, M. Gonzalez, 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-Versille, S. Loucatos, S. Marnieros, S. Masi, S. Scully, S. Spinelli, T.D. Hoang, T. Louis, V. Gilles, W. Marty, Y. Giraud-Heraud","submitted_at":"2021-01-17T21:20:07Z","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 laboratory in Paris (APC). The detection chain is currently made of 256 NbSi transition edge sensors (TES) cooled to 320 mK. The readout system is a 128:1 time domain multiplexing scheme based on 128 SQUIDs cooled at 1 K that are controlled and amplified by an SiGe application specific integrated circuit at 40 K. We report the performance of this readout chain and the characterization of the TES. The readout system has been fu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.06787","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/2101.06787/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"}