BICEP array cryostat and mount design
International audience Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style receivers that compose the Keck Array with four larger Bicep3 style receivers observing at six f...
Published in: | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX |
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Online Access: | https://hal.science/hal-01851187 https://doi.org/10.1117/12.2312829 |
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ftunivnantes:oai:HAL:hal-01851187v1 2023-05-15T18:22:25+02:00 BICEP array cryostat and mount design Crumrine, Michael Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S.A. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Kang, J.H. 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.V. Megerian, K.G. Moncelsi, L. Namikawa, T. Nguyen, H.T. O'Brient, R. Ogburn, R.W. Palladino, S. Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Austin, United States 2018-06-10 https://hal.science/hal-01851187 https://doi.org/10.1117/12.2312829 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/1808.00569 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2312829 hal-01851187 https://hal.science/hal-01851187 ARXIV: 1808.00569 doi:10.1117/12.2312829 INSPIRE: 1682443 Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2018 https://hal.science/hal-01851187 SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082D, ⟨10.1117/12.2312829⟩ Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP Keck Array Cosmology cosmic background radiation: polarization detector: cryogenics gravitational radiation: primordial cosmological model synchrotron detector: performance galaxy [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/10.1117/12.2312829 2023-03-08T06:08:29Z International audience Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style receivers that compose the Keck Array with four larger Bicep3 style receivers observing at six frequencies from 30 to 270GHz. The 95GHz and 150GHz receivers will continue to push the already deep Bicep/Keck CMB maps while the 30/40GHz and 220/270GHz receivers will constrain the synchrotron and galactic dust foregrounds respectively. Here we report on the design and performance of the Bicep Array instruments focusing on the mount and cryostat systems. Conference Object South pole Université de Nantes: HAL-UNIV-NANTES Austin South Pole Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 83 |
institution |
Open Polar |
collection |
Université de Nantes: HAL-UNIV-NANTES |
op_collection_id |
ftunivnantes |
language |
English |
topic |
Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP Keck Array Cosmology cosmic background radiation: polarization detector: cryogenics gravitational radiation: primordial cosmological model synchrotron detector: performance galaxy [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 BICEP Keck Array Cosmology cosmic background radiation: polarization detector: cryogenics gravitational radiation: primordial cosmological model synchrotron detector: performance galaxy [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Crumrine, Michael Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S.A. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Kang, J.H. 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.V. Megerian, K.G. Moncelsi, L. Namikawa, T. Nguyen, H.T. O'Brient, R. Ogburn, R.W. Palladino, S. BICEP array cryostat and mount design |
topic_facet |
Cosmic Microwave Background Inflation Gravitational Waves Polarization BICEP Keck Array Cosmology cosmic background radiation: polarization detector: cryogenics gravitational radiation: primordial cosmological model synchrotron detector: performance galaxy [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 Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style receivers that compose the Keck Array with four larger Bicep3 style receivers observing at six frequencies from 30 to 270GHz. The 95GHz and 150GHz receivers will continue to push the already deep Bicep/Keck CMB maps while the 30/40GHz and 220/270GHz receivers will constrain the synchrotron and galactic dust foregrounds respectively. Here we report on the design and performance of the Bicep Array instruments focusing on the mount and cryostat systems. |
author2 |
Commissariat à l'énergie atomique et aux énergies alternatives (CEA) |
format |
Conference Object |
author |
Crumrine, Michael Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S.A. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Kang, J.H. 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.V. Megerian, K.G. Moncelsi, L. Namikawa, T. Nguyen, H.T. O'Brient, R. Ogburn, R.W. Palladino, S. |
author_facet |
Crumrine, Michael Ade, P.A. R. Ahmed, Z. Aikin, R.W. Alexander, K.D. Barkats, D. Benton, S.J. Bischoff, C.A. Bock, J.J. Bowens-Rubin, R. Brevik, J.A. Buder, I. Bullock, E. Buza, V. Connors, J. Cornelison, J. Crill, B.P. Dierickx, M. Duband, L. Dvorkin, C. Filippini, J.P. Fliescher, S. Grayson, J.A. Hall, G. Halpern, M. Harrison, S.A. Hildebrandt, S.R. Hilton, G.C. Hui, H. Irwin, K.D. Kang, J.H. 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.V. Megerian, K.G. Moncelsi, L. Namikawa, T. Nguyen, H.T. O'Brient, R. Ogburn, R.W. Palladino, S. |
author_sort |
Crumrine, Michael |
title |
BICEP array cryostat and mount design |
title_short |
BICEP array cryostat and mount design |
title_full |
BICEP array cryostat and mount design |
title_fullStr |
BICEP array cryostat and mount design |
title_full_unstemmed |
BICEP array cryostat and mount design |
title_sort |
bicep array cryostat and mount design |
publisher |
HAL CCSD |
publishDate |
2018 |
url |
https://hal.science/hal-01851187 https://doi.org/10.1117/12.2312829 |
op_coverage |
Austin, United States |
geographic |
Austin South Pole |
geographic_facet |
Austin 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-01851187 SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.107082D, ⟨10.1117/12.2312829⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/1808.00569 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2312829 hal-01851187 https://hal.science/hal-01851187 ARXIV: 1808.00569 doi:10.1117/12.2312829 INSPIRE: 1682443 |
op_doi |
https://doi.org/10.1117/12.2312829 |
container_title |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX |
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83 |
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1766201838057553920 |