QUBIC Experiment Toward the First Light
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 c...
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| Autor*in: |
D’Alessandro, G. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Dordrecht : Springer Science + Business Media B.V., 1969, 209(2022), 5-6 vom: 10. Aug., Seite 839-848 |
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| Übergeordnetes Werk: |
volume:209 ; year:2022 ; number:5-6 ; day:10 ; month:08 ; pages:839-848 |
| Links: |
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| DOI / URN: |
10.1007/s10909-022-02775-z |
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| Katalog-ID: |
SPR048771163 |
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| 520 | |a 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. | ||
| 650 | 4 | |a Instruments: mm-wave |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Applications: astrophysics and cosmology |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Battistelli, E. S. |4 aut | |
| 700 | 1 | |a de Bernardis, P. |4 aut | |
| 700 | 1 | |a De Petris, M. |4 aut | |
| 700 | 1 | |a Gamboa Lerena, M. M. |4 aut | |
| 700 | 1 | |a Grandsire, L. |4 aut | |
| 700 | 1 | |a Hamilton, J.-Ch. |4 aut | |
| 700 | 1 | |a Marnieros, S. |4 aut | |
| 700 | 1 | |a Masi, S. |4 aut | |
| 700 | 1 | |a Mennella, A. |4 aut | |
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| 700 | 1 | |a O’Sullivan, C. |4 aut | |
| 700 | 1 | |a Piat, M. |4 aut | |
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| 700 | 1 | |a Alberro, J. G. |4 aut | |
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| 700 | 1 | |a Bersanelli, M. |4 aut | |
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10.1007/s10909-022-02775-z doi (DE-627)SPR048771163 (SPR)s10909-022-02775-z-e DE-627 ger DE-627 rakwb eng D’Alessandro, G. verfasserin (orcid)0000-0002-2580-043X aut QUBIC Experiment Toward the First Light 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. 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. Instruments: mm-wave (dpeaa)DE-He213 Applications: astrophysics and cosmology (dpeaa)DE-He213 Battistelli, E. S. aut de Bernardis, P. aut De Petris, M. aut Gamboa Lerena, M. M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Marnieros, S. aut Masi, S. aut Mennella, A. aut Mousset, L. aut O’Sullivan, C. aut Piat, M. aut Tartari, A. aut Torchinsky, S. A. aut Voisin, F. aut Zannoni, M. aut Ade, P. aut Alberro, J. G. aut Almela, A. aut Amico, G. aut Arnaldi, L. H. aut Auguste, D. aut Aumont, J. aut Azzoni, S. aut Banfi, S. aut Baù, A. aut Bélier, B. aut Bennett, D. aut Bergé, L. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Cavaliere, F. aut Chanial, P. aut Chapron, C. aut Charlassier, R. aut Cobos Cerutti, A. C. aut Columbro, F. aut Coppolecchia, A. aut De Gasperis, G. aut De Leo, M. aut Dheilly, S. aut Duca, C. aut Dumoulin, L. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Ganga, K. M. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut González, M. aut Gradziel, M. aut Hampel, M. R. aut Harari, D. aut Henrot-Versillé, S. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Maffei, B. aut Marty, W. aut Mattei, A. aut May, A. aut McCulloch, M. aut Mele, L. aut Melo, D. aut Montier, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut Olivieri, E. aut Oriol, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perbost, C. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Prêle, D. aut Presta, G. aut Puddu, R. aut Rambaud, D. aut Rasztocky, E. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. G. aut Scully, S. aut Spinelli, S. aut Stankowiak, G. aut Stolpovskiy, M. aut Supanitsky, A. D. aut Thermeau, J.-P. aut Timbie, P. aut Tomasi, M. aut Tucker, G. aut Tucker, C. aut Viganò, D. aut Vittorio, N. aut Wicek, F. aut Wright, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 209(2022), 5-6 vom: 10. Aug., Seite 839-848 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:209 year:2022 number:5-6 day:10 month:08 pages:839-848 https://dx.doi.org/10.1007/s10909-022-02775-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 209 2022 5-6 10 08 839-848 |
| spelling |
10.1007/s10909-022-02775-z doi (DE-627)SPR048771163 (SPR)s10909-022-02775-z-e DE-627 ger DE-627 rakwb eng D’Alessandro, G. verfasserin (orcid)0000-0002-2580-043X aut QUBIC Experiment Toward the First Light 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. 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. Instruments: mm-wave (dpeaa)DE-He213 Applications: astrophysics and cosmology (dpeaa)DE-He213 Battistelli, E. S. aut de Bernardis, P. aut De Petris, M. aut Gamboa Lerena, M. M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Marnieros, S. aut Masi, S. aut Mennella, A. aut Mousset, L. aut O’Sullivan, C. aut Piat, M. aut Tartari, A. aut Torchinsky, S. A. aut Voisin, F. aut Zannoni, M. aut Ade, P. aut Alberro, J. G. aut Almela, A. aut Amico, G. aut Arnaldi, L. H. aut Auguste, D. aut Aumont, J. aut Azzoni, S. aut Banfi, S. aut Baù, A. aut Bélier, B. aut Bennett, D. aut Bergé, L. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Cavaliere, F. aut Chanial, P. aut Chapron, C. aut Charlassier, R. aut Cobos Cerutti, A. C. aut Columbro, F. aut Coppolecchia, A. aut De Gasperis, G. aut De Leo, M. aut Dheilly, S. aut Duca, C. aut Dumoulin, L. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Ganga, K. M. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut González, M. aut Gradziel, M. aut Hampel, M. R. aut Harari, D. aut Henrot-Versillé, S. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Maffei, B. aut Marty, W. aut Mattei, A. aut May, A. aut McCulloch, M. aut Mele, L. aut Melo, D. aut Montier, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut Olivieri, E. aut Oriol, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perbost, C. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Prêle, D. aut Presta, G. aut Puddu, R. aut Rambaud, D. aut Rasztocky, E. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. G. aut Scully, S. aut Spinelli, S. aut Stankowiak, G. aut Stolpovskiy, M. aut Supanitsky, A. D. aut Thermeau, J.-P. aut Timbie, P. aut Tomasi, M. aut Tucker, G. aut Tucker, C. aut Viganò, D. aut Vittorio, N. aut Wicek, F. aut Wright, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 209(2022), 5-6 vom: 10. Aug., Seite 839-848 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:209 year:2022 number:5-6 day:10 month:08 pages:839-848 https://dx.doi.org/10.1007/s10909-022-02775-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 209 2022 5-6 10 08 839-848 |
| allfields_unstemmed |
10.1007/s10909-022-02775-z doi (DE-627)SPR048771163 (SPR)s10909-022-02775-z-e DE-627 ger DE-627 rakwb eng D’Alessandro, G. verfasserin (orcid)0000-0002-2580-043X aut QUBIC Experiment Toward the First Light 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. 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. Instruments: mm-wave (dpeaa)DE-He213 Applications: astrophysics and cosmology (dpeaa)DE-He213 Battistelli, E. S. aut de Bernardis, P. aut De Petris, M. aut Gamboa Lerena, M. M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Marnieros, S. aut Masi, S. aut Mennella, A. aut Mousset, L. aut O’Sullivan, C. aut Piat, M. aut Tartari, A. aut Torchinsky, S. A. aut Voisin, F. aut Zannoni, M. aut Ade, P. aut Alberro, J. G. aut Almela, A. aut Amico, G. aut Arnaldi, L. H. aut Auguste, D. aut Aumont, J. aut Azzoni, S. aut Banfi, S. aut Baù, A. aut Bélier, B. aut Bennett, D. aut Bergé, L. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Cavaliere, F. aut Chanial, P. aut Chapron, C. aut Charlassier, R. aut Cobos Cerutti, A. C. aut Columbro, F. aut Coppolecchia, A. aut De Gasperis, G. aut De Leo, M. aut Dheilly, S. aut Duca, C. aut Dumoulin, L. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Ganga, K. M. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut González, M. aut Gradziel, M. aut Hampel, M. R. aut Harari, D. aut Henrot-Versillé, S. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Maffei, B. aut Marty, W. aut Mattei, A. aut May, A. aut McCulloch, M. aut Mele, L. aut Melo, D. aut Montier, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut Olivieri, E. aut Oriol, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perbost, C. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Prêle, D. aut Presta, G. aut Puddu, R. aut Rambaud, D. aut Rasztocky, E. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. G. aut Scully, S. aut Spinelli, S. aut Stankowiak, G. aut Stolpovskiy, M. aut Supanitsky, A. D. aut Thermeau, J.-P. aut Timbie, P. aut Tomasi, M. aut Tucker, G. aut Tucker, C. aut Viganò, D. aut Vittorio, N. aut Wicek, F. aut Wright, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 209(2022), 5-6 vom: 10. Aug., Seite 839-848 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:209 year:2022 number:5-6 day:10 month:08 pages:839-848 https://dx.doi.org/10.1007/s10909-022-02775-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 209 2022 5-6 10 08 839-848 |
| allfieldsGer |
10.1007/s10909-022-02775-z doi (DE-627)SPR048771163 (SPR)s10909-022-02775-z-e DE-627 ger DE-627 rakwb eng D’Alessandro, G. verfasserin (orcid)0000-0002-2580-043X aut QUBIC Experiment Toward the First Light 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. 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. Instruments: mm-wave (dpeaa)DE-He213 Applications: astrophysics and cosmology (dpeaa)DE-He213 Battistelli, E. S. aut de Bernardis, P. aut De Petris, M. aut Gamboa Lerena, M. M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Marnieros, S. aut Masi, S. aut Mennella, A. aut Mousset, L. aut O’Sullivan, C. aut Piat, M. aut Tartari, A. aut Torchinsky, S. A. aut Voisin, F. aut Zannoni, M. aut Ade, P. aut Alberro, J. G. aut Almela, A. aut Amico, G. aut Arnaldi, L. H. aut Auguste, D. aut Aumont, J. aut Azzoni, S. aut Banfi, S. aut Baù, A. aut Bélier, B. aut Bennett, D. aut Bergé, L. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Cavaliere, F. aut Chanial, P. aut Chapron, C. aut Charlassier, R. aut Cobos Cerutti, A. C. aut Columbro, F. aut Coppolecchia, A. aut De Gasperis, G. aut De Leo, M. aut Dheilly, S. aut Duca, C. aut Dumoulin, L. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Ganga, K. M. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut González, M. aut Gradziel, M. aut Hampel, M. R. aut Harari, D. aut Henrot-Versillé, S. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Maffei, B. aut Marty, W. aut Mattei, A. aut May, A. aut McCulloch, M. aut Mele, L. aut Melo, D. aut Montier, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut Olivieri, E. aut Oriol, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perbost, C. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Prêle, D. aut Presta, G. aut Puddu, R. aut Rambaud, D. aut Rasztocky, E. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. G. aut Scully, S. aut Spinelli, S. aut Stankowiak, G. aut Stolpovskiy, M. aut Supanitsky, A. D. aut Thermeau, J.-P. aut Timbie, P. aut Tomasi, M. aut Tucker, G. aut Tucker, C. aut Viganò, D. aut Vittorio, N. aut Wicek, F. aut Wright, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 209(2022), 5-6 vom: 10. Aug., Seite 839-848 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:209 year:2022 number:5-6 day:10 month:08 pages:839-848 https://dx.doi.org/10.1007/s10909-022-02775-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 209 2022 5-6 10 08 839-848 |
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10.1007/s10909-022-02775-z doi (DE-627)SPR048771163 (SPR)s10909-022-02775-z-e DE-627 ger DE-627 rakwb eng D’Alessandro, G. verfasserin (orcid)0000-0002-2580-043X aut QUBIC Experiment Toward the First Light 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. 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. Instruments: mm-wave (dpeaa)DE-He213 Applications: astrophysics and cosmology (dpeaa)DE-He213 Battistelli, E. S. aut de Bernardis, P. aut De Petris, M. aut Gamboa Lerena, M. M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Marnieros, S. aut Masi, S. aut Mennella, A. aut Mousset, L. aut O’Sullivan, C. aut Piat, M. aut Tartari, A. aut Torchinsky, S. A. aut Voisin, F. aut Zannoni, M. aut Ade, P. aut Alberro, J. G. aut Almela, A. aut Amico, G. aut Arnaldi, L. H. aut Auguste, D. aut Aumont, J. aut Azzoni, S. aut Banfi, S. aut Baù, A. aut Bélier, B. aut Bennett, D. aut Bergé, L. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Cavaliere, F. aut Chanial, P. aut Chapron, C. aut Charlassier, R. aut Cobos Cerutti, A. C. aut Columbro, F. aut Coppolecchia, A. aut De Gasperis, G. aut De Leo, M. aut Dheilly, S. aut Duca, C. aut Dumoulin, L. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Ganga, K. M. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut González, M. aut Gradziel, M. aut Hampel, M. R. aut Harari, D. aut Henrot-Versillé, S. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Maffei, B. aut Marty, W. aut Mattei, A. aut May, A. aut McCulloch, M. aut Mele, L. aut Melo, D. aut Montier, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut Olivieri, E. aut Oriol, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perbost, C. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Prêle, D. aut Presta, G. aut Puddu, R. aut Rambaud, D. aut Rasztocky, E. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. G. aut Scully, S. aut Spinelli, S. aut Stankowiak, G. aut Stolpovskiy, M. aut Supanitsky, A. D. aut Thermeau, J.-P. aut Timbie, P. aut Tomasi, M. aut Tucker, G. aut Tucker, C. aut Viganò, D. aut Vittorio, N. aut Wicek, F. aut Wright, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Dordrecht : Springer Science + Business Media B.V., 1969 209(2022), 5-6 vom: 10. Aug., Seite 839-848 (DE-627)320575411 (DE-600)2016984-X 1573-7357 nnns volume:209 year:2022 number:5-6 day:10 month:08 pages:839-848 https://dx.doi.org/10.1007/s10909-022-02775-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 209 2022 5-6 10 08 839-848 |
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D’Alessandro, G. @@aut@@ Battistelli, E. S. @@aut@@ de Bernardis, P. @@aut@@ De Petris, M. @@aut@@ Gamboa Lerena, M. M. @@aut@@ Grandsire, L. @@aut@@ Hamilton, J.-Ch. @@aut@@ Marnieros, S. @@aut@@ Masi, S. @@aut@@ Mennella, A. @@aut@@ Mousset, L. @@aut@@ O’Sullivan, C. @@aut@@ Piat, M. @@aut@@ Tartari, A. @@aut@@ Torchinsky, S. A. @@aut@@ Voisin, F. @@aut@@ Zannoni, M. @@aut@@ Ade, P. @@aut@@ Alberro, J. G. @@aut@@ Almela, A. @@aut@@ Amico, G. @@aut@@ Arnaldi, L. H. @@aut@@ Auguste, D. @@aut@@ Aumont, J. @@aut@@ Azzoni, S. @@aut@@ Banfi, S. @@aut@@ Baù, A. @@aut@@ Bélier, B. @@aut@@ Bennett, D. @@aut@@ Bergé, L. @@aut@@ Bernard, J.-Ph. @@aut@@ Bersanelli, M. @@aut@@ Bigot-Sazy, M.-A. @@aut@@ Bonaparte, J. @@aut@@ Bonis, J. @@aut@@ Bunn, E. @@aut@@ Burke, D. @@aut@@ Buzi, D. @@aut@@ Cavaliere, F. @@aut@@ Chanial, P. @@aut@@ Chapron, C. @@aut@@ Charlassier, R. @@aut@@ Cobos Cerutti, A. C. @@aut@@ Columbro, F. @@aut@@ Coppolecchia, A. @@aut@@ De Gasperis, G. @@aut@@ De Leo, M. @@aut@@ Dheilly, S. @@aut@@ Duca, C. @@aut@@ Dumoulin, L. @@aut@@ Etchegoyen, A. @@aut@@ Fasciszewski, A. @@aut@@ Ferreyro, L. P. @@aut@@ Fracchia, D. @@aut@@ Franceschet, C. @@aut@@ Ganga, K. M. @@aut@@ García, B. @@aut@@ García Redondo, M. E. @@aut@@ Gaspard, M. @@aut@@ Gayer, D. @@aut@@ Gervasi, M. @@aut@@ Giard, M. @@aut@@ Gilles, V. @@aut@@ Giraud-Heraud, Y. @@aut@@ Gómez Berisso, M. @@aut@@ González, M. @@aut@@ Gradziel, M. @@aut@@ Hampel, M. R. @@aut@@ Harari, D. @@aut@@ Henrot-Versillé, S. @@aut@@ Incardona, F. @@aut@@ Jules, E. @@aut@@ Kaplan, J. @@aut@@ Kristukat, C. @@aut@@ Lamagna, L. @@aut@@ Loucatos, S. @@aut@@ Louis, T. @@aut@@ Maffei, B. @@aut@@ Marty, W. @@aut@@ Mattei, A. @@aut@@ May, A. @@aut@@ McCulloch, M. @@aut@@ Mele, L. @@aut@@ Melo, D. @@aut@@ Montier, L. @@aut@@ Mundo, L. M. @@aut@@ Murphy, J. A. @@aut@@ Murphy, J. D. @@aut@@ Nati, F. @@aut@@ Olivieri, E. @@aut@@ Oriol, C. @@aut@@ Paiella, A. @@aut@@ Pajot, F. @@aut@@ Passerini, A. @@aut@@ Pastoriza, H. @@aut@@ Pelosi, A. @@aut@@ Perbost, C. @@aut@@ Perciballi, M. @@aut@@ Pezzotta, F. @@aut@@ Piacentini, F. @@aut@@ Piccirillo, L. @@aut@@ Pisano, G. @@aut@@ Platino, M. @@aut@@ Polenta, G. @@aut@@ Prêle, D. @@aut@@ Presta, G. @@aut@@ Puddu, R. @@aut@@ Rambaud, D. @@aut@@ Rasztocky, E. @@aut@@ Ringegni, P. @@aut@@ Romero, G. E. @@aut@@ Salum, J. M. @@aut@@ Schillaci, A. @@aut@@ Scóccola, C. G. @@aut@@ Scully, S. @@aut@@ Spinelli, S. @@aut@@ Stankowiak, G. @@aut@@ Stolpovskiy, M. @@aut@@ Supanitsky, A. D. @@aut@@ Thermeau, J.-P. @@aut@@ Timbie, P. @@aut@@ Tomasi, M. @@aut@@ Tucker, G. @@aut@@ Tucker, C. @@aut@@ Viganò, D. @@aut@@ Vittorio, N. @@aut@@ Wicek, F. @@aut@@ Wright, M. @@aut@@ Zullo, A. @@aut@@ |
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D’Alessandro, G. Battistelli, E. S. de Bernardis, P. De Petris, M. Gamboa Lerena, M. M. Grandsire, L. Hamilton, J.-Ch. Marnieros, S. Masi, S. Mennella, A. Mousset, L. O’Sullivan, C. Piat, M. Tartari, A. Torchinsky, S. A. Voisin, F. Zannoni, M. Ade, P. Alberro, J. G. Almela, A. Amico, G. Arnaldi, L. H. Auguste, D. Aumont, J. Azzoni, S. Banfi, S. Baù, A. Bélier, B. Bennett, D. Bergé, L. Bernard, J.-Ph. Bersanelli, M. Bigot-Sazy, M.-A. Bonaparte, J. Bonis, J. Bunn, E. Burke, D. Buzi, D. Cavaliere, F. Chanial, P. Chapron, C. Charlassier, R. Cobos Cerutti, A. C. Columbro, F. Coppolecchia, A. De Gasperis, G. De Leo, M. Dheilly, S. Duca, C. Dumoulin, L. Etchegoyen, A. Fasciszewski, A. Ferreyro, L. P. Fracchia, D. Franceschet, C. Ganga, K. M. García, B. García Redondo, M. E. Gaspard, M. Gayer, D. Gervasi, M. Giard, M. Gilles, V. Giraud-Heraud, Y. Gómez Berisso, M. González, M. Gradziel, M. Hampel, M. R. Harari, D. Henrot-Versillé, S. Incardona, F. Jules, E. Kaplan, J. Kristukat, C. Lamagna, L. Loucatos, S. Louis, T. Maffei, B. Marty, W. Mattei, A. May, A. McCulloch, M. Mele, L. Melo, D. Montier, L. Mundo, L. M. Murphy, J. A. Murphy, J. D. Nati, F. Olivieri, E. Oriol, C. Paiella, A. Pajot, F. Passerini, A. Pastoriza, H. Pelosi, A. Perbost, C. Perciballi, M. Pezzotta, F. Piacentini, F. Piccirillo, L. Pisano, G. Platino, M. Polenta, G. Prêle, D. Presta, G. Puddu, R. Rambaud, D. Rasztocky, E. Ringegni, P. Romero, G. E. Salum, J. M. Schillaci, A. Scóccola, C. G. Scully, S. Spinelli, S. Stankowiak, G. Stolpovskiy, M. Supanitsky, A. D. Thermeau, J.-P. Timbie, P. Tomasi, M. Tucker, G. Tucker, C. Viganò, D. Vittorio, N. Wicek, F. Wright, M. Zullo, A. |
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QUBIC Experiment Toward the First Light |
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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. © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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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. © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
| abstract_unstemmed |
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. © The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR048771163</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230509121602.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">221201s2022 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10909-022-02775-z</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR048771163</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s10909-022-02775-z-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">D’Alessandro, G.</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(orcid)0000-0002-2580-043X</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">QUBIC Experiment Toward the First Light</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2022</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Author(s), under exclusive licence to Springer Science+Business Media, LLC, part of Springer Nature 2022. Springer Nature or its licensor holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">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. 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