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Status of QUBIC, the Q&U Bolometer for Cosmology

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arxiv 2210.03161 v1 pith:W7WEGHDN submitted 2022-10-06 astro-ph.IM astro-ph.CO

L. Mousset , P. Ade , A. Almela , G. Amico , L.H. Arnaldi , J. Aumont , S. Banfi , E.S. Battistelli
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B. Bélier L. Bergé J.-Ph. Bernard P. de Bernardis M. Bersanelli J. Bonaparte J.D. Bonilla E. Bunn D. Buzi D. Camilieri F. Cavaliere P. Chanial C. Chapron S. Colombo F. Columbro A. Coppolecchia B. Costanza G. DÁlessandro G. De Gasperis M. De Leo M. De Petris N. Del Castillo S. Dheilly A. Etchegoyen M. Famá L.P. Ferreyro C. Franceschet M.M. Gamboa Lerena K.M. Ganga B. García M.E. García Redondo D. Gayer J.M. Geria M. Gervasi M. Giard V. Gilles M. Gómez Berisso M. González M. Gradziel L. Grandsire J.-Ch. Hamilton M.R. Hampel G. Isopi J. Kaplan C. Kristukat L. Lamagna F. Lazarte S. Loucatos A. Mancilla D. Mandelli E. Manzan S. Marnieros W. Marty S. Masi A. May J. Maya M. McCulloch L. Mele D. Melo A. Mennella N. Mirón-Granese L. Montier N. Müller J.D. Murphy F. Nati C. OŚullivan A. Paiella F. Pajot S.Paradiso A. Passerini A.Pelosi M. Perciballi F. Pezzotta F. Piacentini M. Piat L. Piccirillo G. Pisano M. Platino G. Polenta D. Prêle D. Rambaud E. Rasztocky M. Régnier C. Reyes F. Rodríguez C.A. Rodríguez G.E. Romero J.M. Salum A. Schillaci C.G. Scóccola G. Stankowiak A.D. Supanitsky A. Tartari J.-P. Thermeau P. Timbie S.A. Torchinsky G. Tucker C. Tucker L. Vacher F. Voisin M. Wright M. Zannoni A. Zullo
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classification astro-ph.IMastro-ph.CO
keywords cosmologyqubicbolometricinstrumentalnovelobservationaltermsaddress
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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.

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