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QUBIC Technological Design Report

Authors :
Aumont, J.
Banfi, S.
Battaglia, P.
Battistelli, E. S.
Baù, A.
Bélier, B.
Bennett, D.
Bergé, L.
Ph Bernard, J.
Bersanelli, M.
Bigot-Sazy, M. A.
Bleurvacq, N.
Bordier, G.
Brossard, J.
Bunn, E. F.
Buzi, D.
Buzzelli, A.
Cammilleri, D.
Cavaliere, F.
Chanial, P.
Chapron, C.
Coppi, G.
Coppolecchia, A.
François Couchot
Agostino, R. D.
Alessandro, G. D.
Bernardis, P.
Gasperis, G.
Petris, M.
Decourcelle, T.
Del Torto, F.
Dumoulin, L.
Etchegoyen, A.
Franceschet, C.
Garcia, B.
Gault, A.
Gayer, D.
Gervasi, M.
Ghribi, A.
Giard, M.
Giraud-Héraud, Y.
Gradziel, M.
Grandsire, L.
Ch Hamilton, J.
Harari, D.
Haynes, V.
Henrot-Versillé, S.
Holtzer, N.
Kaplan, J.
Korotkov, A.
Lande, J.
Loucatos, S.
Lowitz, A.
Lukovic, V.
Maffei, B.
Marnieros, S.
Martino, J.
Masi, S.
Medina, M. C.
Mcculloch, M.
May, A.
Melhuish, S.
Mennella, A.
Montier, L.
Murphy, A.
Néel, D.
Ng, M. W.
Sullivan, C. O.
Pajot, F.
Passerini, A.
Pelosi, A.
Perbost, C.
Perdereau, O.
Piacentini, F.
Piat, M.
Piccirillo, L.
Pisano, G.
Prêle, D.
Puddu, R.
Rambaud, D.
Rigaut, O.
Romero, G. E.
Salatino, M.
Schillaci, A.
Scully, S.
Stolpovskiy, M.
Tartari, A.
Timbie, P.
Tristram, M.
Tucker, G.
Viganò, D.
Vittori, N.
Voisin, F.
Watson, B.
Zannoni, M.
Zullo, A.
Laboratoire de l'Accélérateur Linéaire (LAL)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Q&U Bolometric Interferometer for Cosmology
QUBIC
Source :
[Technical Report] Q&U Bolometric Interferometer for Cosmology. 2016, HAL
Publication Year :
2016
Publisher :
HAL CCSD, 2016.

Abstract

139 pages ; high resolution version can be found on the qubic website (http://qubic.in2p3.fr/QUBIC/Home.html); QUBIC is an instrument aiming at measuring the B mode polarisation anisotropies at medium scales angular scales (30-200 multipoles). The search for the primordial CMB B-mode polarization signal is challenging, because of many difficulties: smallness of the expected signal, instrumental systematics that could possibly induce polarization leakage from the large E signal into B, brighter than anticipated polarized foregrounds (dust) reducing to zero the initial hope of finding sky regions clean enough to have a direct primordial B-modes observation. The QUBIC instrument is designed to address all aspects of this challenge with a novel kind of instrument, a Bolometric Interferometer, combining the background-limited sensitivity of Transition-Edge-Sensors and the control of systematics allowed by the observation of interference fringe patterns, while operating at two frequencies to disentangle polarized foregrounds from primordial B mode polarization. Its characteristics are described in details in this Technological Design Report.

Details

Language :
English
Database :
OpenAIRE
Journal :
[Technical Report] Q&U Bolometric Interferometer for Cosmology. 2016, HAL
Accession number :
edsair.dedup.wf.001..5f2772eb2090066021ad7ddbfa30d89f