2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization
International audience BICEP3 is a 520mm aperture on-axis refracting telescope observing the polarization of the cosmic microwave background (CMB) at 95GHz in search of the B-mode signal originating from in ationary gravitational waves. BICEP3's focal plane is populated with modularized tiles o...
Published in: | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX |
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Format: | Conference Object |
Language: | English |
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Online Access: | https://hal.science/hal-01851180 https://doi.org/10.1117/12.2313854 |
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ftunivnantes:oai:HAL:hal-01851180v1 2023-05-15T18:22:42+02:00 2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization Kang, Jae Hwan Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Boenish, H. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Crumrine, M. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Karkare, K.S. Karpel, E. Kaufman, J.P. Keating, B.G. Kefeli, S. Kernasovskiy, S.A. Kovac, J.M. Kuo, C.L. Lau, K. Larsen, N.A. Leitch, E.M. Lueker, M. Megerian, K.G. Moncelsi, L. Namikawa, T. Netterfield, B. Nguyen, H.T. O'Brient, R. Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Austin, United States 2018-06-10 https://hal.science/hal-01851180 https://doi.org/10.1117/12.2313854 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/1808.00567 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2313854 hal-01851180 https://hal.science/hal-01851180 ARXIV: 1808.00567 doi:10.1117/12.2313854 INSPIRE: 1682450 Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2018 https://hal.science/hal-01851180 SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082N, ⟨10.1117/12.2313854⟩ Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP3 Keck Array cosmic background radiation: polarization beam: width detector: performance detector: upgrade cosmic background radiation: B-mode noise gravitational radiation: primordial bolometer optics [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2018 ftunivnantes https://doi.org/10.1117/12.2313854 2023-03-08T06:08:29Z International audience BICEP3 is a 520mm aperture on-axis refracting telescope observing the polarization of the cosmic microwave background (CMB) at 95GHz in search of the B-mode signal originating from in ationary gravitational waves. BICEP3's focal plane is populated with modularized tiles of antenna-coupled transition edge sensor (TES) bolometers. BICEP3 was deployed to the South Pole during 2014-15 austral summer and has been operational since. During the 2016-17 austral summer, we implemented changes to optical elements that lead to better noise performance. We discuss this upgrade and show the performance of BICEP3 at its full mapping speed from the 2017 and 2018 observing seasons. BICEP3 achieves an order-of-magnitude improvement in mapping speed compared to a Keck 95GHz receiver. We demonstrate 6.6μK√s noise performance of the BICEP3 receiver. Conference Object South pole Université de Nantes: HAL-UNIV-NANTES Austin Austral South Pole Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 93 |
institution |
Open Polar |
collection |
Université de Nantes: HAL-UNIV-NANTES |
op_collection_id |
ftunivnantes |
language |
English |
topic |
Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP3 Keck Array cosmic background radiation: polarization beam: width detector: performance detector: upgrade cosmic background radiation: B-mode noise gravitational radiation: primordial bolometer optics [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP3 Keck Array cosmic background radiation: polarization beam: width detector: performance detector: upgrade cosmic background radiation: B-mode noise gravitational radiation: primordial bolometer optics [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Kang, Jae Hwan Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Boenish, H. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Crumrine, M. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Karkare, K.S. Karpel, E. Kaufman, J.P. Keating, B.G. Kefeli, S. Kernasovskiy, S.A. Kovac, J.M. Kuo, C.L. Lau, K. Larsen, N.A. Leitch, E.M. Lueker, M. Megerian, K.G. Moncelsi, L. Namikawa, T. Netterfield, B. Nguyen, H.T. O'Brient, R. 2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
topic_facet |
Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP3 Keck Array cosmic background radiation: polarization beam: width detector: performance detector: upgrade cosmic background radiation: B-mode noise gravitational radiation: primordial bolometer optics [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience BICEP3 is a 520mm aperture on-axis refracting telescope observing the polarization of the cosmic microwave background (CMB) at 95GHz in search of the B-mode signal originating from in ationary gravitational waves. BICEP3's focal plane is populated with modularized tiles of antenna-coupled transition edge sensor (TES) bolometers. BICEP3 was deployed to the South Pole during 2014-15 austral summer and has been operational since. During the 2016-17 austral summer, we implemented changes to optical elements that lead to better noise performance. We discuss this upgrade and show the performance of BICEP3 at its full mapping speed from the 2017 and 2018 observing seasons. BICEP3 achieves an order-of-magnitude improvement in mapping speed compared to a Keck 95GHz receiver. We demonstrate 6.6μK√s noise performance of the BICEP3 receiver. |
author2 |
Commissariat à l'énergie atomique et aux énergies alternatives (CEA) |
format |
Conference Object |
author |
Kang, Jae Hwan Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Boenish, H. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Crumrine, M. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Karkare, K.S. Karpel, E. Kaufman, J.P. Keating, B.G. Kefeli, S. Kernasovskiy, S.A. Kovac, J.M. Kuo, C.L. Lau, K. Larsen, N.A. Leitch, E.M. Lueker, M. Megerian, K.G. Moncelsi, L. Namikawa, T. Netterfield, B. Nguyen, H.T. O'Brient, R. |
author_facet |
Kang, Jae Hwan Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Boenish, H. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Crumrine, M. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Karkare, K.S. Karpel, E. Kaufman, J.P. Keating, B.G. Kefeli, S. Kernasovskiy, S.A. Kovac, J.M. Kuo, C.L. Lau, K. Larsen, N.A. Leitch, E.M. Lueker, M. Megerian, K.G. Moncelsi, L. Namikawa, T. Netterfield, B. Nguyen, H.T. O'Brient, R. |
author_sort |
Kang, Jae Hwan |
title |
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
title_short |
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
title_full |
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
title_fullStr |
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
title_full_unstemmed |
2017 upgrade and performance of BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization |
title_sort |
2017 upgrade and performance of bicep3: a 95ghz refracting telescope for degree-scale cmb polarization |
publisher |
HAL CCSD |
publishDate |
2018 |
url |
https://hal.science/hal-01851180 https://doi.org/10.1117/12.2313854 |
op_coverage |
Austin, United States |
geographic |
Austin Austral South Pole |
geographic_facet |
Austin Austral South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2018 https://hal.science/hal-01851180 SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082N, ⟨10.1117/12.2313854⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/1808.00567 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2313854 hal-01851180 https://hal.science/hal-01851180 ARXIV: 1808.00567 doi:10.1117/12.2313854 INSPIRE: 1682450 |
op_doi |
https://doi.org/10.1117/12.2313854 |
container_title |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX |
container_start_page |
93 |
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1766202115707895808 |