QUBIC: The Q & U Bolometric Interferometer for Cosmology
Creators
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Battistelli, E. S.1, 2
- Ade, P.3
- Alberro, J. G.4
- Almela, A.5
- Amico, G.1
- Arnaldi, L. H.6
- Auguste, D.7
- Aumont, J.8
- Azzoni, S.9
- Banfi, S.10, 11
- Battaglia, P.12
- Baù, A.10, 11
- Bélier, B.13
- Bennett, D.14
- Bergé, L.7
- Bernard, J.-Ph.8
- Bersanelli, M.12
- Bigot-Sazy, M.-A.15
- Bleurvacq, N.15
- Bonaparte, J.6
- Bonis, J.7
- Bottani, A.4
- Bunn, E.16
- Burke, D.14
- Buzi, D.1
- Buzzelli, A.17
- Cavaliere, F.12
- Chanial, P.15
- Chapron, C.15
- Charlassier, R.15
- Columbro, F.1, 2
- Coppi, G.9
- Coppolecchia, A.1, 2
- D'Alessandro, G.1, 2
- de Bernardis, P.1, 2
- De Gasperis, G.17
- De Leo, M.1, 18
- De Petris, M.1, 2
- Dheilly, S.15
- Di Donato, A.6
- Dumoulin, L.7
- Etchegoyen, A.5
- Fasciszewski, A.6
- Ferreyro, L. P.5
- Fracchia, D.5
- Franceschet, C.12
- Gamboa Lerena, M. M.4
- Ganga, K.15
- García, B.5
- García Redondo, M. E.5
- Gaspard, M.7
- Gault, A.19
- Gayer, D.14
- Gervasi, M.10, 11
- Giard, M.8
- Gilles, V.1
- Giraud-Heraud, Y.15
- Gómez Berisso, M.6
- González, M.6
- Gradziel, M.14
- Grandsire, L.15
- Hamilton, J.-Ch.15
- Harari, D.6
- Haynes, V.9
- Henrot-Versillé, S.7
- Hoang, D. T.15
- Incardona, F.12
- Jules, E.7
- Kaplan, J.15
- Korotkov, A.20
- Kristukat, C.6, 21
- Lamagna, L.1, 2
- Loucatos, S.15
- Louis, T.7
- Luterstein, R.6
- Maffei, B.22
- Marnieros, S.7
- Marty, W.8
- Masi, S.1, 2
- Mattei, A.2
- May, A.9
- McCulloch, M.9
- Medina, M. C.23
- Mele, L.1, 2
- Melhuish, S.9
- Mennella, A.12
- Montier, L.8
- Mousset, L.15
- Mundo, L. M.4
- Murphy, J. A.14
- Murphy, J. D.14
- Nati, F.10, 11
- Olivieri, E.7
- Oriol, C.7
- O'Sullivan, C.14
- Paiella, A.1, 2
- Pajot, F.8
- Passerini, A.10, 11
- Pastoriza, H.6
- Pelosi, A.2
- Perbost, C.15
- Perciballi, M.2
- Pezzotta, F.12
- Piacentini, F.1, 2
- Piat, M.15
- Piccirillo, L.9
- Pisano, G.3
- Platino, M.5
- Polenta, G.24
- Prêle, D.15
- Puddu, R.25
- Rambaud, D.8
- Ringegni, P.4
- Romero, G. E.23
- Salatino, M.26
- Salum, J. M.5
- Schillaci, A.27
- Scóccola, C.4
- Scully, S.14
- Spinelli, S.10
- Stankowiak, G.15
- Stolpovskiy, M.15
- Suarez, F.5
- Tartari, A.28
- Thermeau, J.-P.15
- Timbie, P.19
- Tomasi, M.12
- Torchinsky, S.15
- Tristram, M.7
- Tucker, C.3
- Tucker, G.20
- Vanneste, S.7
- Viganò, D.12
- Vittorio, N.17
- Voisin, F.15
- Watson, B.9
- Wicek, F.7
- Zannoni, M.10, 11
- Zullo, A.2
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1.
Sapienza University of Rome
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2.
INFN Sezione di Roma I
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3.
Cardiff University
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4.
National University of La Plata
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5.
Instituto de Tecnologías en Detección y Astropartículas
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6.
Comisión Nacional de Energía Atómica
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7.
Laboratoire de Physique des 2 Infinis Irène Joliot-Curie
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8.
Research Institute in Astrophysics and Planetology
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9.
University of Manchester
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10.
University of Milano-Bicocca
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11.
INFN Sezione di Milano
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12.
University of Milan
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13.
Centre for Nanoscience and Nanotechnology
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14.
National University of Ireland, Maynooth
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15.
Astroparticle and Cosmology Laboratory
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16.
University of Richmond
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17.
University of Rome Tor Vergata
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18.
University of Surrey
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19.
University of Wisconsin–Madison
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20.
Brown University
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21.
National University of General San Martín
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22.
Institut d'Astrophysique Spatiale
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23.
Instituto Argentino de Radioastronomía
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24.
Agenzia Spaziale Italiana
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25.
Pontificia Universidad Católica de Chile
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26.
Kavli Institute for Particle Astrophysics and Cosmology
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27.
California Institute of Technology
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28.
INFN Sezione di Pisa
Abstract
The Q & U Bolometric Interferometer for Cosmology, QUBIC, is an innovative experiment designed to measure the polarization of the cosmic microwave background and in particular the signature left therein by the inflationary expansion of the Universe. The expected signal is extremely faint; thus, extreme sensitivity and systematic control are necessary in order to attempt this measurement. QUBIC addresses these requirements using an innovative approach combining the sensitivity of transition-edge sensor cryogenic bolometers, with the deep control of systematics characteristic of interferometers. This makes QUBIC unique with respect to others' classical imagers experiments devoted to the CMB polarization. In this contribution, we report a description of the QUBIC instrument including recent achievements and the demonstration of the bolometric interferometry performed in laboratory. QUBIC will be deployed at the observation site in Alto Chorrillos, in Argentina, at the end of 2019.
Additional Information
© 2020 Springer-Verlag. Received 31 July 2019; Accepted 27 January 2020; Published 24 February 2020. QUBIC is funded by the following agencies. France: ANR (Agence Nationale de la Recherche) 2012 and 2014, DIM-ACAV (Domaine d'Interet Majeur-Astronomie et Conditions d'Apparition de la Vie), CNRS/IN2P3 (Centre national de la recherche scientifique/Institut national de physique nucleáire et de physique des particules), CNRS/INSU (Centre national de la recherche scientifique/Institut national de sciences de l'univers). Italy: CNR/PNRA (Consiglio Nazionale delle Ricerche/Programma Nazionale Ricerche in Antartide) until 2016, INFN (Istituto Nazionale di Fisica Nucleare) since 2017. Argentina: Secretaría de Gobierno de Ciencia, Tecnología e Innovación Productiva, Comisión Nacional de Energía Atómica, Consejo Nacional de Investigaciones Científicas y Técnicas.Attached Files
Submitted - 2001.10272.pdf
Files
2001.10272.pdf
Additional details
Identifiers
- Eprint ID
- 101997
- Resolver ID
- CaltechAUTHORS:20200319-121737388
Related works
- Describes
- https://arxiv.org/abs/2001.10272 (URL)
Funding
- Agence Nationale pour la Recherche (ANR)
- Domaine d'Interet Majeur-Astronomie et Conditions d'Apparition de la Vie
- Centre National de la Recherche Scientifique (CNRS)
- Institut National de Physique Nucléaire et de Physique des Particules (IN2P3)
- Consiglio Nazionale delle Ricerche (CNR)
- Programma Nazionale Ricerche in Antartide (PNRA)
- Istituto Nazionale di Fisica Nucleare (INFN)
- Secretaría de Gobierno de Ciencia, Tecnología e Innovación Productiva
- Comisión Nacional de Energía Atómica
- Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET)
Dates
- Created
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2020-03-19Created from EPrint's datestamp field
- Updated
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2023-03-16Created from EPrint's last_modified field