QUBIC: Measuring CMB polarization from Argentina

de Bernardis, P, Ade, P ORCID: https://orcid.org/0000-0002-5127-0401, Amico, G, Auguste, D, Aumont, J, Banfi, S, Barbarán, G, Battaglia, P, Battistelli, E, Baù, A, Bélier, B, Bennett, D, Bergé, L, Bernard, J.P, Bersanelli, M, Bigot-Sazy, M.A, Bleurvacq, N, Bonaparte, J, Bonis, J, Bordier, G, Bréelle, E, Bunn, E, Burke, D, Buzi, D, Buzzelli, A, Cavaliere, F, Chanial, P, Chapron, C, Charlassier, R, Columbro, F, Coppi, G, Coppolecchia, A, Couchot, F, D'Agostino, R, D'Alessandro, G, De Gasperis, G, De Leo, M, De Petris, M, Di Donato, A, Dumoulin, L, Etchegoyen, A, Fasciszewski, A, Franceschet, C, Gamboa Lerena, M.M, García, B, Garrido, X, Gaspard, M, Gault, A, Gayer, D, Gervasi, M, Giard, M, Giraud-Heraud, Y, Gómez Berisso, M, González, M, Gradziel, M, Grandsire, L, Guerrard, E, Hamilton, J.C, Harari, D, Haynes, V, Henrot-Versillé, S, Hoang, T, Incardona, F, Jules, E, Kaplan, J, Korotkov, A, Kristukat, C, Lamagna, L, Loucatos, S, Louis, T, Lowitz, A, Lukovic, V, Luterstein, R, Maffei, B, Marnieros, S, Masi, S, Mattei, A, May, A, McCulloch, M, Medina, M.C, Mele, L, Melhuish, S, Mennella, A, Montier, L, Mundo, L.M, Murphy, J.A, Murphy, J.D, Olivieri, E, O'Sullivan, C, Paiella, A, Pajot, F, Passerini, A, Pastoriza, H, Pelosi, A, Perbost, C, Perdereau, O, Pezzotta, F, Piacentini, F, Piat, M, Piccirillo, L, Pisano, G ORCID: https://orcid.org/0000-0003-4302-5681, Polenta, G, Prêle, D, Puddu, R, Rambaud, D, Ringegni, P, Romero, G.E, Salatino, M, Schillaci, A, Scóccola, C, Scully, S, Spinelli, S, Stolpovskiy, M, Suarez, F, Tartari, A, Thermeau, J.P, Timbie, P, Torchinsky, S, Tristram, M, Truongcanh, V, Tucker, G, Tucker, C ORCID: https://orcid.org/0000-0002-1851-3918, Vanneste, S, Viganò, D, Vittorio, N, Voisin, F, Watson, B, Wicek, F, Zannoni, M and Zullo, A 2018. QUBIC: Measuring CMB polarization from Argentina. Boletín de la Asociación Argentina de Astronomía 60 , pp. 107-114.

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Abstract

QUBIC (Q and U Bolometric Interferometer for Cosmology) is an ambitious project to measure the polarization of the Cosmic Microwave Background (CMB), which can provide unique information on the very early universe and the cosmic inflation process. The QUBIC instrument combines the extreme sensitivity of cryogenic bolometers and the accurate control of beam-forming and auto-calibration ability of interferometers. The instrument is being finalized and calibrated for a first installation at the Alto Chorrillo high altitude site (Salta province, Argentina) in late 2018, and will produce, in the first two years of operation, a sensitive measurement of CMB polarization, able to detect a tensor to scalar ratio for B-modes 0.01....

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Physics and Astronomy
Last Modified:	28 Apr 2023 13:46
URI:	https://orca.cardiff.ac.uk/id/eprint/156827

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