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QUBIC instrument for CMB polarization measurements

Mele, L. and Ade, P. and Alberro, J. G. and Almela, A. and Amico, G. and Arnaldi, L. H. and Auguste, D. and Aumont, J. and Azzoni, S. and Banfi, S. and Battistelli, E. S. and Baù, A. and Bèlier, B. and Bennett, D. and Bergé, L. and Bernard, J.-Ph. and Bersanelli, M. and Bigot-Sazy, M.-A. and Bleurvacq, N. and Bonaparte, J. and Bonis, J. and Bottani, A. and Bunn, E. and Burke, D. and Buzi, D. and Cavaliere, F. and Chanial, P. and Chapron, C. and Charlassier, R. and Columbro, F. and Coppolecchia, A. and D’Alessandro, G. and de Bernardis, P. and De Gasperis, G. and De Leo, M. and De Petris, M. and Dheilly, S. and Dumoulin, L. and Etchegoyen, A. and Fasciszewski, A. and Ferreyro, L. P. and Fracchia, D. and Franceschet, C. and Gamboa Lerena, M. M. and Ganga, K. and García, B. and García Redondo, M. E. and Gaspard, M. and Gayer, D. and Gervasi, M. and Giard, M. and Gilles, V. and Giraud-Heraud, Y. and Gómez Berisso, M. and González, M. and Gradziel, M. and Grandsire, L. and Hamilton, J.-Ch. and Harari, D. and Henrot-Versillé, S. and Hoang, D. T. and Incardona, F. and Jules, E. and Kaplan, J. and Kristukat, C. and Lamagna, L. and Loucatos, S. and Louis, T. and Maffei, B. and Marnieros, S. and Marty, W. and Masi, S. and Mattei, A. and May, A. and McCulloch, M. and Melhuish, S. and Mennella, A. and Montier, L. and Mousset, L. and Mundo, L. M. and Murphy, J. A. and Murphy, J. D. and Nati, F. and Olivieri, E. and Oriol, C. and O’Sullivan, C. and Paiella, A. and Pajot, F. and Passerini, A. and Pastoriza, H. and Pelosi, A. and Perbost, C. and Perciballi, M. and Pezzotta, F. and Piacentini, F. and Piat, M. and Piccirillo, L. and Pisano, G. and Platino, M. and Polenta, G. and Prêle, D. and Puddu, R. and Rambaud, D. and Ringegni, P. and Romero, G. E. and Salatino, M. and Salum, J. M. and Schillaci, A. and Scóccola, C. and Scully, S. and Spinelli, S. and Stankowiak, G. and Stolpovskiy, M. and Tartari, A. and Thermeau, J.-P. and Timbie, P. and Tomasi, M. and Torchinsky, S. and Tristram, M. and Tucker, G. and Tucker, C. and Viganò, D. and Vittorio, N. and Voisin, F. and Wicek, F. and Zannoni, M. and Zullo, A. (2020) QUBIC instrument for CMB polarization measurements. Journal of Physics Conference Series, 1548 . Art. No. 012016. ISSN 1742-6588. https://resolver.caltech.edu/CaltechAUTHORS:20200922-072635843

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Abstract

Measurements of cosmic microwave background (CMB) polarization may reveal the presence of a background of gravitational waves produced during cosmic inflation, providing thus a test of inflationary models. The Q&U Bolometric Interferometer for Cosmology (QUBIC) is an experiment designed to measure the CMB polarization. It is based on the novel concept of bolometric interferometry, which combines the sensitivity of bolometric detectors with the properties of beam synthesis and control of calibration offered by interferometers. To modulate and extract the input polarized signal of the CMB, QUBIC exploits Stokes polarimetry based on a rotating half-wave plate (HWP). In this work, we illustrate the design of the QUBIC instrument, focusing on the polarization modulation system, and we present preliminary results of beam calibrations and the performance of the HWP rotator at 300 K.


Item Type:Article
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https://doi.org/10.1088/1742-6596/1548/1/012016DOIArticle
Additional Information:© 2020 Published under licence by IOP Publishing Ltd. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Record Number:CaltechAUTHORS:20200922-072635843
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200922-072635843
Official Citation:L Mele et al 2020 J. Phys.: Conf. Ser. 1548 012016
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:105465
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:22 Sep 2020 16:52
Last Modified:22 Sep 2020 16:52

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