학술논문
Status of QUBIC, the Q&U Bolometer for Cosmology
Document Type
Working Paper
Author
Mousset, L.; Ade, P.; Almela, A.; Amico, G.; Arnaldi, L. H.; Aumont, J.; Banfi, S.; Battistelli, E. S.; Bélier, B.; Bergé, L.; Bernard, J. -Ph.; de Bernardis, P.; Bersanelli, M.; Bonaparte, J.; Bonilla, J. D.; Bunn, E.; Buzi, D.; Camilieri, D.; Cavaliere, F.; Chanial, P.; Chapron, C.; Colombo, S.; Columbro, F.; Coppolecchia, A.; Costanza, B.; DÁlessandro, G.; De Gasperis, G.; De Leo, M.; De Petris, M.; Del Castillo, N.; Dheilly, S.; Etchegoyen, A.; Famá, M.; Ferreyro, L. P.; Franceschet, C.; Lerena, M. M. Gamboa; Ganga, K. M.; García, B.; Redondo, M. E. García; Gayer, D.; Geria, J. M.; Gervasi, M.; Giard, M.; Gilles, V.; Berisso, M. Gómez; González, M.; Gradziel, M.; Grandsire, L.; Hamilton, J. -Ch.; Hampel, M. R.; Isopi, G.; Kaplan, J.; Kristukat, C.; Lamagna, L.; Lazarte, F.; Loucatos, S.; Mancilla, A.; Mandelli, D.; Manzan, E.; Marnieros, S.; Marty, W.; Masi, S.; May, A.; Maya, J.; McCulloch, M.; Mele, L.; Melo, D.; Mennella, A.; Mirón-Granese, N.; Montier, L.; Müller, N.; Murphy, J. D.; Nati, F.; OŚullivan, C.; Paiella, A.; Pajot, F.; Paradiso, S.; Passerini, A.; Pelosi, A.; Perciballi, M.; Pezzotta, F.; Piacentini, F.; Piat, M.; Piccirillo, L.; Pisano, G.; Platino, M.; Polenta, G.; Prêle, D.; Rambaud, D.; Rasztocky, E.; Régnier, M.; Reyes, C.; Rodríguez, F.; Rodríguez, C. A.; Romero, G. E.; Salum, J. M.; Schillaci, A.; Scóccola, C. G.; Stankowiak, G.; Supanitsky, A. D.; Tartari, A.; Thermeau, J. -P.; Timbie, P.; Torchinsky, S. A.; Tucker, G.; Tucker, C.; Vacher, L.; Voisin, F.; Wright, M.; Zannoni, M.; Zullo, A.
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Subject
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Abstract
The Q&U Bolometric Interferometer for Cosmology (QUBIC) is a novel kind of polarimeter optimized for the measurement of the B-mode polarization of the Cosmic Microwave Back-ground (CMB), which is one of the major challenges of observational cosmology. The signal is expected to be of the order of a few tens of nK, prone to instrumental systematic effects and polluted by various astrophysical foregrounds which can only be controlled through multichroic observations. QUBIC is designed to address these observational issues with a novel approach that combines the advantages of interferometry in terms of control of instrumental systematics with those of bolometric detectors in terms of wide-band, background-limited sensitivity.
Comment: Contribution to the 2022 Cosmology session of the 33rd Rencontres de Blois. arXiv admin note: substantial text overlap with arXiv:2203.08947
Comment: Contribution to the 2022 Cosmology session of the 33rd Rencontres de Blois. arXiv admin note: substantial text overlap with arXiv:2203.08947