QUBIC Experiment Toward the First Light
Creators
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D'Alessandro, G.1, 2
- Battistelli, E. S.1, 2
- de Bernardis, P.1, 2
- De Petris, M.1, 2
- Gamboa Lerena, M. M.3, 4
- Grandsire, L.5
- Hamilton, J.-Ch.5
- Marnieros, S.6
- Masi, S.1, 2
- Mennella, A.7, 8
- Mousset, L.5
- O'Sullivan, C.9
- Piat, M.5
- Tartari, A.10
- Torchinsky, S. A.5, 11
- Voisin, F.5
- Zannoni, M.12, 13
- Ade, P.14
- Alberro, J. G.3
- Almela, A.15
- Amico, G.1
- Arnaldi, L. H.16
- Auguste, D.6
- Aumont, J.17
- Azzoni, S.18
- Banfi, S.12, 13
- Baù, A.12, 13
- Bélier, B.19
- Bennett, D.9
- Bergé, L.6
- Bernard, J.-Ph.17
- Bersanelli, M.7, 8
- Bigot-Sazy, M.-A.5
- Bonaparte, J.
- Bonis, J.6
- Bunn, E.20
- Burke, D.9
- Buzi, D.1
- Cavaliere, F.7, 8
- Chanial, P.5
- Chapron, C.5
- Charlassier, R.5
- Cobos Cerutti, A. C.15
- Columbro, F.1, 2
- Coppolecchia, A.1, 2
- De Gasperis, G.21, 22
- De Leo, M.1, 23
- Dheilly, S.5
- Duca, C.15
- Dumoulin, L.6
- Etchegoyen, A.15
- Fasciszewski, A.
- Ferreyro, L. P.15
- Fracchia, D.15
- Franceschet, C.7, 8
- Ganga, K. M.5
- García, B.15
- García Redondo, M. E.15
- Gaspard, M.6
- Gayer, D.9
- Gervasi, M.12, 13
- Giard, M.17
- Gilles, V.1, 24
- Giraud-Heraud, Y.5
- Gómez Berisso, M.16
- González, M.16
- Gradziel, M.9
- Hampel, M. R.15
- Harari, D.16
- Henrot-Versillé, S.6
- Incardona, F.7, 8
- Jules, E.6
- Kaplan, J.5
- Kristukat, C.
- Lamagna, L.1, 2
- Loucatos, S.5, 25
- Louis, T.6
- Maffei, B.26
- Marty, W.17
- Mattei, A.2
- May, A.24
- McCulloch, M.24
- Mele, L.1, 2
- Melo, D.15
- Montier, L.17
- Mundo, L. M.3
- Murphy, J. A.9
- Murphy, J. D.9
- Nati, F.12, 13
- Olivieri, E.6
- Oriol, C.6
- Paiella, A.1, 2
- Pajot, F.17
- Passerini, A.12, 13
- Pastoriza, H.16
- Pelosi, A.2
- Perbost, C.5
- Perciballi, M.2
- Pezzotta, F.7, 8
- Piacentini, F.1, 2
- Piccirillo, L.24
- Pisano, G.1, 14
- Platino, M.15
- Polenta, G.1, 27
- Prêle, D.5
- Presta, G.1, 2
- Puddu, R.1, 28
- Rambaud, D.17
- Rasztocky, E.29
- Ringegni, P.3
- Romero, G. E.29
- Salum, J. M.15
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Schillaci, A.1, 30
- Scóccola, C. G.3, 4
- Scully, S.9
- Spinelli, S.12
- Stankowiak, G.5
- Stolpovskiy, M.5
- Supanitsky, A. D.15
- Thermeau, J.-P.5
- Timbie, P.31
- Tomasi, M.7, 8
- Tucker, G.32
- Tucker, C.14
- Viganò, D.7, 8
- Vittorio, N.21
- Wicek, F.6
- Wright, M.24
- 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.
National University of La Plata
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4.
National Scientific and Technical Research Council
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5.
Astroparticle and Cosmology Laboratory
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6.
Laboratoire de Physique des 2 Infinis Irène Joliot-Curie
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7.
University of Milan
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8.
INFN Sezione di Milano
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9.
National University of Ireland, Maynooth
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10.
INFN Sezione di Pisa
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11.
Paris Observatory
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12.
University of Milano-Bicocca
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13.
INFN Sezione di Milano Bicocca
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14.
Cardiff University
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15.
Instituto de Tecnologías en Detección y Astropartículas
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16.
Bariloche Atomic Centre
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17.
Research Institute in Astrophysics and Planetology
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18.
University of Oxford
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19.
Centre for Nanoscience and Nanotechnology
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20.
University of Richmond
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21.
University of Rome Tor Vergata
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22.
National Institute for Nuclear Physics
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23.
University of Surrey
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24.
University of Manchester
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25.
Institut de Recherche sur les Lois Fondamentales de l'Univers
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26.
Institut d'Astrophysique Spatiale
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27.
Agenzia Spaziale Italiana
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28.
Pontificia Universidad Católica de Chile
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29.
Centro de Investigaciones Cardiovasculares
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30.
California Institute of Technology
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31.
University of Wisconsin–Madison
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32.
Brown University
Abstract
The Q & U Bolometric Interferometer for Cosmology (QUBIC) is a cosmology experiment that aims to measure the B-mode polarization of the cosmic microwave background (CMB). Measurements of the primordial B-mode pattern of the CMB polarization are in fact among the most exciting goals in cosmology as it would allow testing of the inflationary paradigm. Many experiments are attempting to measure the B-modes, from the ground and the stratosphere, using imaging Stokes polarimeters. The QUBIC collaboration developed an innovative concept to measure CMB polarization using bolometric interferometry. This approach mixes the high sensitivity of bolometric detectors with the accurate control of systematics due to the interferometric layout of the instrument. We present the calibration results for the Technological Demonstrator, before its commissioning in the Argentinian observing site and preparation for first light.
Additional details
Identifiers
- Eprint ID
- 116402
- Resolver ID
- CaltechAUTHORS:20220823-625642500.752
Dates
- Created
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2022-08-26Created from EPrint's datestamp field
- Updated
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2023-03-16Created from EPrint's last_modified field