QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB
Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the i...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Piat, M. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Springer US, 1969, 200(2020), 5-6 vom: 27. Apr., Seite 363-373 |
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| Übergeordnetes Werk: |
volume:200 ; year:2020 ; number:5-6 ; day:27 ; month:04 ; pages:363-373 |
| Links: |
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| DOI / URN: |
10.1007/s10909-020-02445-y |
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| Katalog-ID: |
OLC2119356297 |
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| 520 | |a Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. | ||
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10.1007/s10909-020-02445-y doi (DE-627)OLC2119356297 (DE-He213)s10909-020-02445-y-p DE-627 ger DE-627 rakwb eng 530 VZ Piat, M. verfasserin aut QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. TESs TDM CMB Bélier, B. aut Bergé, L. aut Bleurvacq, N. aut Chapron, C. aut Dheilly, S. aut Dumoulin, L. aut González, M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Henrot-Versillé, S. aut Hoang, D. T. aut Marnieros, S. aut Marty, W. aut Montier, L. aut Olivieri, E. aut Oriol, C. aut Perbost, C. aut Prêle, D. aut Rambaud, D. aut Salatino, M. aut Stankowiak, G. aut Thermeau, J.-P. aut Torchinsky, S. aut Voisin, F. 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 Battaglia, P. aut Battistelli, E. S. aut Baù, A. aut Bennett, D. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bottani, A. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Buzzelli, A. aut Cavaliere, F. aut Chanial, P. aut Charlassier, R. aut Columbro, F. aut Coppi, G. aut Coppolecchia, A. aut D’Alessandro, G. aut de Bernardis, P. aut De Gasperis, G. aut De Leo, M. aut De Petris, M. aut Di Donato, A. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Gamboa Lerena, M. M. aut Ganga, K. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gault, A. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut Gradziel, M. aut Harari, D. aut Haynes, V. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Korotkov, A. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Luterstein, R. aut Maffei, B. aut Masi, S. aut Mattei, A. aut May, A. aut McCulloch, M. aut Medina, M. C. aut Mele, L. aut Melhuish, S. aut Mennella, A. aut Mousset, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut O’Sullivan, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Puddu, R. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. aut Scully, S. aut Spinelli, S. aut Stolpovskiy, M. aut Suarez, F. aut Tartari, A. aut Timbie, P. aut Tomasi, M. aut Tucker, C. aut Tucker, G. aut Vanneste, S. aut Viganò, D. aut Vittorio, N. aut Watson, B. aut Wicek, F. aut Zannoni, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Springer US, 1969 200(2020), 5-6 vom: 27. Apr., Seite 363-373 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:200 year:2020 number:5-6 day:27 month:04 pages:363-373 https://doi.org/10.1007/s10909-020-02445-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_4126 AR 200 2020 5-6 27 04 363-373 |
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10.1007/s10909-020-02445-y doi (DE-627)OLC2119356297 (DE-He213)s10909-020-02445-y-p DE-627 ger DE-627 rakwb eng 530 VZ Piat, M. verfasserin aut QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. TESs TDM CMB Bélier, B. aut Bergé, L. aut Bleurvacq, N. aut Chapron, C. aut Dheilly, S. aut Dumoulin, L. aut González, M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Henrot-Versillé, S. aut Hoang, D. T. aut Marnieros, S. aut Marty, W. aut Montier, L. aut Olivieri, E. aut Oriol, C. aut Perbost, C. aut Prêle, D. aut Rambaud, D. aut Salatino, M. aut Stankowiak, G. aut Thermeau, J.-P. aut Torchinsky, S. aut Voisin, F. 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 Battaglia, P. aut Battistelli, E. S. aut Baù, A. aut Bennett, D. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bottani, A. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Buzzelli, A. aut Cavaliere, F. aut Chanial, P. aut Charlassier, R. aut Columbro, F. aut Coppi, G. aut Coppolecchia, A. aut D’Alessandro, G. aut de Bernardis, P. aut De Gasperis, G. aut De Leo, M. aut De Petris, M. aut Di Donato, A. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Gamboa Lerena, M. M. aut Ganga, K. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gault, A. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut Gradziel, M. aut Harari, D. aut Haynes, V. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Korotkov, A. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Luterstein, R. aut Maffei, B. aut Masi, S. aut Mattei, A. aut May, A. aut McCulloch, M. aut Medina, M. C. aut Mele, L. aut Melhuish, S. aut Mennella, A. aut Mousset, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut O’Sullivan, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Puddu, R. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. aut Scully, S. aut Spinelli, S. aut Stolpovskiy, M. aut Suarez, F. aut Tartari, A. aut Timbie, P. aut Tomasi, M. aut Tucker, C. aut Tucker, G. aut Vanneste, S. aut Viganò, D. aut Vittorio, N. aut Watson, B. aut Wicek, F. aut Zannoni, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Springer US, 1969 200(2020), 5-6 vom: 27. Apr., Seite 363-373 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:200 year:2020 number:5-6 day:27 month:04 pages:363-373 https://doi.org/10.1007/s10909-020-02445-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_4126 AR 200 2020 5-6 27 04 363-373 |
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10.1007/s10909-020-02445-y doi (DE-627)OLC2119356297 (DE-He213)s10909-020-02445-y-p DE-627 ger DE-627 rakwb eng 530 VZ Piat, M. verfasserin aut QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. TESs TDM CMB Bélier, B. aut Bergé, L. aut Bleurvacq, N. aut Chapron, C. aut Dheilly, S. aut Dumoulin, L. aut González, M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Henrot-Versillé, S. aut Hoang, D. T. aut Marnieros, S. aut Marty, W. aut Montier, L. aut Olivieri, E. aut Oriol, C. aut Perbost, C. aut Prêle, D. aut Rambaud, D. aut Salatino, M. aut Stankowiak, G. aut Thermeau, J.-P. aut Torchinsky, S. aut Voisin, F. 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 Battaglia, P. aut Battistelli, E. S. aut Baù, A. aut Bennett, D. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bottani, A. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Buzzelli, A. aut Cavaliere, F. aut Chanial, P. aut Charlassier, R. aut Columbro, F. aut Coppi, G. aut Coppolecchia, A. aut D’Alessandro, G. aut de Bernardis, P. aut De Gasperis, G. aut De Leo, M. aut De Petris, M. aut Di Donato, A. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Gamboa Lerena, M. M. aut Ganga, K. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gault, A. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut Gradziel, M. aut Harari, D. aut Haynes, V. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Korotkov, A. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Luterstein, R. aut Maffei, B. aut Masi, S. aut Mattei, A. aut May, A. aut McCulloch, M. aut Medina, M. C. aut Mele, L. aut Melhuish, S. aut Mennella, A. aut Mousset, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut O’Sullivan, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Puddu, R. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. aut Scully, S. aut Spinelli, S. aut Stolpovskiy, M. aut Suarez, F. aut Tartari, A. aut Timbie, P. aut Tomasi, M. aut Tucker, C. aut Tucker, G. aut Vanneste, S. aut Viganò, D. aut Vittorio, N. aut Watson, B. aut Wicek, F. aut Zannoni, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Springer US, 1969 200(2020), 5-6 vom: 27. Apr., Seite 363-373 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:200 year:2020 number:5-6 day:27 month:04 pages:363-373 https://doi.org/10.1007/s10909-020-02445-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_4126 AR 200 2020 5-6 27 04 363-373 |
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10.1007/s10909-020-02445-y doi (DE-627)OLC2119356297 (DE-He213)s10909-020-02445-y-p DE-627 ger DE-627 rakwb eng 530 VZ Piat, M. verfasserin aut QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. TESs TDM CMB Bélier, B. aut Bergé, L. aut Bleurvacq, N. aut Chapron, C. aut Dheilly, S. aut Dumoulin, L. aut González, M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Henrot-Versillé, S. aut Hoang, D. T. aut Marnieros, S. aut Marty, W. aut Montier, L. aut Olivieri, E. aut Oriol, C. aut Perbost, C. aut Prêle, D. aut Rambaud, D. aut Salatino, M. aut Stankowiak, G. aut Thermeau, J.-P. aut Torchinsky, S. aut Voisin, F. 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 Battaglia, P. aut Battistelli, E. S. aut Baù, A. aut Bennett, D. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bottani, A. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Buzzelli, A. aut Cavaliere, F. aut Chanial, P. aut Charlassier, R. aut Columbro, F. aut Coppi, G. aut Coppolecchia, A. aut D’Alessandro, G. aut de Bernardis, P. aut De Gasperis, G. aut De Leo, M. aut De Petris, M. aut Di Donato, A. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Gamboa Lerena, M. M. aut Ganga, K. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gault, A. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut Gradziel, M. aut Harari, D. aut Haynes, V. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Korotkov, A. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Luterstein, R. aut Maffei, B. aut Masi, S. aut Mattei, A. aut May, A. aut McCulloch, M. aut Medina, M. C. aut Mele, L. aut Melhuish, S. aut Mennella, A. aut Mousset, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut O’Sullivan, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Puddu, R. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. aut Scully, S. aut Spinelli, S. aut Stolpovskiy, M. aut Suarez, F. aut Tartari, A. aut Timbie, P. aut Tomasi, M. aut Tucker, C. aut Tucker, G. aut Vanneste, S. aut Viganò, D. aut Vittorio, N. aut Watson, B. aut Wicek, F. aut Zannoni, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Springer US, 1969 200(2020), 5-6 vom: 27. Apr., Seite 363-373 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:200 year:2020 number:5-6 day:27 month:04 pages:363-373 https://doi.org/10.1007/s10909-020-02445-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_4126 AR 200 2020 5-6 27 04 363-373 |
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10.1007/s10909-020-02445-y doi (DE-627)OLC2119356297 (DE-He213)s10909-020-02445-y-p DE-627 ger DE-627 rakwb eng 530 VZ Piat, M. verfasserin aut QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. TESs TDM CMB Bélier, B. aut Bergé, L. aut Bleurvacq, N. aut Chapron, C. aut Dheilly, S. aut Dumoulin, L. aut González, M. aut Grandsire, L. aut Hamilton, J.-Ch. aut Henrot-Versillé, S. aut Hoang, D. T. aut Marnieros, S. aut Marty, W. aut Montier, L. aut Olivieri, E. aut Oriol, C. aut Perbost, C. aut Prêle, D. aut Rambaud, D. aut Salatino, M. aut Stankowiak, G. aut Thermeau, J.-P. aut Torchinsky, S. aut Voisin, F. 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 Battaglia, P. aut Battistelli, E. S. aut Baù, A. aut Bennett, D. aut Bernard, J.-Ph. aut Bersanelli, M. aut Bigot-Sazy, M.-A. aut Bonaparte, J. aut Bonis, J. aut Bottani, A. aut Bunn, E. aut Burke, D. aut Buzi, D. aut Buzzelli, A. aut Cavaliere, F. aut Chanial, P. aut Charlassier, R. aut Columbro, F. aut Coppi, G. aut Coppolecchia, A. aut D’Alessandro, G. aut de Bernardis, P. aut De Gasperis, G. aut De Leo, M. aut De Petris, M. aut Di Donato, A. aut Etchegoyen, A. aut Fasciszewski, A. aut Ferreyro, L. P. aut Fracchia, D. aut Franceschet, C. aut Gamboa Lerena, M. M. aut Ganga, K. aut García, B. aut García Redondo, M. E. aut Gaspard, M. aut Gault, A. aut Gayer, D. aut Gervasi, M. aut Giard, M. aut Gilles, V. aut Giraud-Heraud, Y. aut Gómez Berisso, M. aut Gradziel, M. aut Harari, D. aut Haynes, V. aut Incardona, F. aut Jules, E. aut Kaplan, J. aut Korotkov, A. aut Kristukat, C. aut Lamagna, L. aut Loucatos, S. aut Louis, T. aut Luterstein, R. aut Maffei, B. aut Masi, S. aut Mattei, A. aut May, A. aut McCulloch, M. aut Medina, M. C. aut Mele, L. aut Melhuish, S. aut Mennella, A. aut Mousset, L. aut Mundo, L. M. aut Murphy, J. A. aut Murphy, J. D. aut Nati, F. aut O’Sullivan, C. aut Paiella, A. aut Pajot, F. aut Passerini, A. aut Pastoriza, H. aut Pelosi, A. aut Perciballi, M. aut Pezzotta, F. aut Piacentini, F. aut Piccirillo, L. aut Pisano, G. aut Platino, M. aut Polenta, G. aut Puddu, R. aut Ringegni, P. aut Romero, G. E. aut Salum, J. M. aut Schillaci, A. aut Scóccola, C. aut Scully, S. aut Spinelli, S. aut Stolpovskiy, M. aut Suarez, F. aut Tartari, A. aut Timbie, P. aut Tomasi, M. aut Tucker, C. aut Tucker, G. aut Vanneste, S. aut Viganò, D. aut Vittorio, N. aut Watson, B. aut Wicek, F. aut Zannoni, M. aut Zullo, A. aut Enthalten in Journal of low temperature physics Springer US, 1969 200(2020), 5-6 vom: 27. Apr., Seite 363-373 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:200 year:2020 number:5-6 day:27 month:04 pages:363-373 https://doi.org/10.1007/s10909-020-02445-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_4126 AR 200 2020 5-6 27 04 363-373 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">OLC2119356297</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504170033.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">230504s2020 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10909-020-02445-y</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2119356297</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10909-020-02445-y-p</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="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Piat, M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020</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">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science+Business Media, LLC, part of Springer Nature 2020</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. 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| author |
Piat, M. |
| spellingShingle |
Piat, M. ddc 530 misc TESs misc TDM misc CMB QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB |
| authorStr |
Piat, M. |
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@@773@@(DE-627)129546267 |
| format |
Article |
| dewey-ones |
530 - Physics |
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Piat, M. Bélier, B. Bergé, L. Bleurvacq, N. Chapron, C. Dheilly, S. Dumoulin, L. González, M. Grandsire, L. Hamilton, J.-Ch. Henrot-Versillé, S. Hoang, D. T. Marnieros, S. Marty, W. Montier, L. Olivieri, E. Oriol, C. Perbost, C. Prêle, D. Rambaud, D. Salatino, M. Stankowiak, G. Thermeau, J.-P. Torchinsky, S. Voisin, F. Ade, P. Alberro, J. G. Almela, A. Amico, G. Arnaldi, L. H. Auguste, D. Aumont, J. Azzoni, S. Banfi, S. Battaglia, P. Battistelli, E. S. Baù, A. Bennett, D. Bernard, J.-Ph. Bersanelli, M. Bigot-Sazy, M.-A. Bonaparte, J. Bonis, J. Bottani, A. Bunn, E. Burke, D. Buzi, D. Buzzelli, A. Cavaliere, F. Chanial, P. Charlassier, R. Columbro, F. Coppi, G. Coppolecchia, A. D’Alessandro, G. de Bernardis, P. De Gasperis, G. De Leo, M. De Petris, M. Di Donato, A. Etchegoyen, A. Fasciszewski, A. Ferreyro, L. P. Fracchia, D. Franceschet, C. Gamboa Lerena, M. M. Ganga, K. García, B. García Redondo, M. E. Gaspard, M. Gault, A. Gayer, D. Gervasi, M. Giard, M. Gilles, V. Giraud-Heraud, Y. Gómez Berisso, M. Gradziel, M. Harari, D. Haynes, V. Incardona, F. Jules, E. Kaplan, J. Korotkov, A. Kristukat, C. Lamagna, L. Loucatos, S. Louis, T. Luterstein, R. Maffei, B. Masi, S. Mattei, A. May, A. McCulloch, M. Medina, M. C. Mele, L. Melhuish, S. Mennella, A. Mousset, L. Mundo, L. M. Murphy, J. A. Murphy, J. D. Nati, F. O’Sullivan, C. Paiella, A. Pajot, F. Passerini, A. Pastoriza, H. Pelosi, A. Perciballi, M. Pezzotta, F. Piacentini, F. Piccirillo, L. Pisano, G. Platino, M. Polenta, G. Puddu, R. Ringegni, P. Romero, G. E. Salum, J. M. Schillaci, A. Scóccola, C. Scully, S. Spinelli, S. Stolpovskiy, M. Suarez, F. Tartari, A. Timbie, P. Tomasi, M. Tucker, C. Tucker, G. Vanneste, S. Viganò, D. Vittorio, N. Watson, B. Wicek, F. Zannoni, M. Zullo, A. |
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QUBIC: Using NbSi TESs with a Bolometric Interferometer to Characterize the Polarization of the CMB |
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Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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Abstract Q & U Bolometric Interferometer for Cosmology (QUBIC) is an international ground-based experiment dedicated in the measurement of the polarized fluctuations of the Cosmic Microwave Background. It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low-temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta Province. The QUBIC detection chain consists in 2048 NbSi transition edge sensors (TESs) cooled to 350 mK.The voltage-biased TESs are read out with time domain multiplexing based on Superconducting QUantum Interference Devices at 1 K and a novel SiGe application-specific integrated circuit at 60 K allowing to reach an unprecedented multiplexing factor equal to 128. The QUBIC experiment is currently being characterized in the laboratory with a reduced number of detectors before upgrading to the full instrument. I will present the last results of this characterization phase with a focus on the detectors and readout system. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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Bélier, B. Bergé, L. Bleurvacq, N. Chapron, C. Dheilly, S. Dumoulin, L. González, M. Grandsire, L. Hamilton, J.-Ch Henrot-Versillé, S. Hoang, D. T. Marnieros, S. Marty, W. Montier, L. Olivieri, E. Oriol, C. Perbost, C. Prêle, D. Rambaud, D. Salatino, M. Stankowiak, G. Thermeau, J.-P. Torchinsky, S. Voisin, F. Ade, P. Alberro, J. G. Almela, A. Amico, G. Arnaldi, L. H. Auguste, D. Aumont, J. Azzoni, S. Banfi, S. Battaglia, P. Battistelli, E. S. Baù, A. Bennett, D. Bernard, J.-Ph Bersanelli, M. Bigot-Sazy, M.-A. Bonaparte, J. Bonis, J. Bottani, A. Bunn, E. Burke, D. Buzi, D. Buzzelli, A. Cavaliere, F. Chanial, P. Charlassier, R. Columbro, F. Coppi, G. Coppolecchia, A. D’Alessandro, G. de Bernardis, P. De Gasperis, G. De Leo, M. De Petris, M. Di Donato, A. Etchegoyen, A. Fasciszewski, A. Ferreyro, L. P. Fracchia, D. Franceschet, C. Gamboa Lerena, M. M. Ganga, K. García, B. García Redondo, M. E. Gaspard, M. Gault, A. Gayer, D. Gervasi, M. Giard, M. Gilles, V. Giraud-Heraud, Y. Gómez Berisso, M. Gradziel, M. Harari, D. Haynes, V. Incardona, F. Jules, E. Kaplan, J. Korotkov, A. Kristukat, C. Lamagna, L. Loucatos, S. Louis, T. Luterstein, R. Maffei, B. Masi, S. Mattei, A. May, A. McCulloch, M. Medina, M. C. Mele, L. Melhuish, S. Mennella, A. Mousset, L. Mundo, L. M. Murphy, J. A. Murphy, J. D. Nati, F. O’Sullivan, C. Paiella, A. Pajot, F. Passerini, A. Pastoriza, H. Pelosi, A. Perciballi, M. Pezzotta, F. Piacentini, F. Piccirillo, L. Pisano, G. Platino, M. Polenta, G. Puddu, R. Ringegni, P. Romero, G. E. Salum, J. M. Schillaci, A. Scóccola, C. Scully, S. Spinelli, S. Stolpovskiy, M. Suarez, F. Tartari, A. Timbie, P. Tomasi, M. Tucker, C. Tucker, G. Vanneste, S. Viganò, D. Vittorio, N. Watson, B. Wicek, F. Zannoni, M. Zullo, A. |
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