BICEP Array: 150 GHz detector module development

International audience The BICEP/Keck Collaboration is currently leading the quest to the highest sensitivity measurements of the polarized CMB anisotropies on degree scale with a series of cryogenic telescopes, of which BICEP Array is the latest Stage-3 upgrade with a total of $\sim32,000$ detector...

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Main Authors: Schillaci, A., Ade, P.A.R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C.A., Beck, D., Bock, J.J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.P., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D., Grayson, J.A., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S.R., Hilton, G.C., Hubmayr, J., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Kefeli, S., Kovac, J.M., Kuo, C.L., Lau, K., Leitch, E.M., Lennox, A., Megerian, K.G., Miller, O.Y., Minutolo, L., Moncelsi, L., Nakato, Y.
Other Authors: Département des Systèmes Basses Températures (DSBT ), Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA)
Format: Conference Object
Language:English
Published: HAL CCSD 2021
Subjects:
Online Access:https://hal.science/hal-03483604
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record_format openpolar
spelling ftunivnantes:oai:HAL:hal-03483604v1 2023-05-15T18:23:21+02:00 BICEP Array: 150 GHz detector module development Schillaci, A. Ade, P.A.R. Ahmed, Z. Amiri, M. Barkats, D. Basu Thakur, R. Bischoff, C.A. Beck, D. Bock, J.J. Buza, V. Cheshire, J. Connors, J. Cornelison, J. Crumrine, M. Cukierman, A. Denison, E. Dierickx, M. Duband, L. Eiben, M. Fatigoni, S. Filippini, J.P. Giannakopoulos, C. Goeckner-Wald, N. Goldfinger, D. Grayson, J.A. Grimes, P. Hall, G. Halal, G. Halpern, M. Hand, E. Harrison, S. Henderson, S. Hildebrandt, S.R. Hilton, G.C. Hubmayr, J. Hui, H. Irwin, K.D. Kang, J. Karkare, K.S. Kefeli, S. Kovac, J.M. Kuo, C.L. Lau, K. Leitch, E.M. Lennox, A. Megerian, K.G. Miller, O.Y. Minutolo, L. Moncelsi, L. Nakato, Y. Département des Systèmes Basses Températures (DSBT ) Institut de Recherche Interdisciplinaire de Grenoble (IRIG) Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA) Online Conference, United States 2021-07-19 https://hal.science/hal-03483604 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2111.14785 hal-03483604 https://hal.science/hal-03483604 ARXIV: 2111.14785 INSPIRE: 1979391 19th International Workshop on Low Temperature Detectors https://hal.science/hal-03483604 19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States detector: cryogenics cryogenics: design cosmic background radiation: anisotropy BICEP buildings upgrade superconductivity sensitivity density amplifier readout pole costs performance fabrication [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 2021 ftunivnantes 2023-03-08T02:18:29Z International audience The BICEP/Keck Collaboration is currently leading the quest to the highest sensitivity measurements of the polarized CMB anisotropies on degree scale with a series of cryogenic telescopes, of which BICEP Array is the latest Stage-3 upgrade with a total of $\sim32,000$ detectors. The instrument comprises 4 receivers spanning 30 to 270 GHz, with the low-frequency 30/40 GHz deployed to the South Pole Station in late 2019. The full complement of receivers is forecast to set the most stringent constraints on the tensor to scalar ratio $r$. Building on these advances, the overarching small-aperture telescope concept is already being used as the reference for further Stage-4 experiment design. In this paper I will present the development of the BICEP Array 150 GHz detector module and its fabrication requirements, with highlights on the high-density time division multiplexing (TDM) design of the cryogenic circuit boards. The low-impedance wiring required between the detectors and the first-stage SQUID amplifiers is crucial to maintain a stiff voltage bias on the detectors. A novel multi-layer FR4 Printed Circuit Board (PCB) with superconducting traces, capable of reading out up to 648 detectors, is presented along with its validation tests. I will also describe an ultra-high density TDM detector module we developed for a CMB-S4-like experiment that allows up to 1,920 detectors to be read out. TDM has been chosen as the detector readout technology for the Cosmic Microwave Background Stage-4 (CMB-S4) experiment based on its proven low-noise performance, predictable costs and overall maturity of the architecture. The heritage for TDM is rooted in mm- and submm-wave experiments dating back 20 years and has since evolved to support a multiplexing factor of 64x in Stage-3 experiments. Conference Object South pole Université de Nantes: HAL-UNIV-NANTES South Pole
institution Open Polar
collection Université de Nantes: HAL-UNIV-NANTES
op_collection_id ftunivnantes
language English
topic detector: cryogenics
cryogenics: design
cosmic background radiation: anisotropy
BICEP
buildings
upgrade
superconductivity
sensitivity
density
amplifier
readout
pole
costs
performance
fabrication
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
spellingShingle detector: cryogenics
cryogenics: design
cosmic background radiation: anisotropy
BICEP
buildings
upgrade
superconductivity
sensitivity
density
amplifier
readout
pole
costs
performance
fabrication
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Schillaci, A.
Ade, P.A.R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Basu Thakur, R.
Bischoff, C.A.
Beck, D.
Bock, J.J.
Buza, V.
Cheshire, J.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A.
Denison, E.
Dierickx, M.
Duband, L.
Eiben, M.
Fatigoni, S.
Filippini, J.P.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D.
Grayson, J.A.
Grimes, P.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S.
Henderson, S.
Hildebrandt, S.R.
Hilton, G.C.
Hubmayr, J.
Hui, H.
Irwin, K.D.
Kang, J.
Karkare, K.S.
Kefeli, S.
Kovac, J.M.
Kuo, C.L.
Lau, K.
Leitch, E.M.
Lennox, A.
Megerian, K.G.
Miller, O.Y.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
BICEP Array: 150 GHz detector module development
topic_facet detector: cryogenics
cryogenics: design
cosmic background radiation: anisotropy
BICEP
buildings
upgrade
superconductivity
sensitivity
density
amplifier
readout
pole
costs
performance
fabrication
[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 The BICEP/Keck Collaboration is currently leading the quest to the highest sensitivity measurements of the polarized CMB anisotropies on degree scale with a series of cryogenic telescopes, of which BICEP Array is the latest Stage-3 upgrade with a total of $\sim32,000$ detectors. The instrument comprises 4 receivers spanning 30 to 270 GHz, with the low-frequency 30/40 GHz deployed to the South Pole Station in late 2019. The full complement of receivers is forecast to set the most stringent constraints on the tensor to scalar ratio $r$. Building on these advances, the overarching small-aperture telescope concept is already being used as the reference for further Stage-4 experiment design. In this paper I will present the development of the BICEP Array 150 GHz detector module and its fabrication requirements, with highlights on the high-density time division multiplexing (TDM) design of the cryogenic circuit boards. The low-impedance wiring required between the detectors and the first-stage SQUID amplifiers is crucial to maintain a stiff voltage bias on the detectors. A novel multi-layer FR4 Printed Circuit Board (PCB) with superconducting traces, capable of reading out up to 648 detectors, is presented along with its validation tests. I will also describe an ultra-high density TDM detector module we developed for a CMB-S4-like experiment that allows up to 1,920 detectors to be read out. TDM has been chosen as the detector readout technology for the Cosmic Microwave Background Stage-4 (CMB-S4) experiment based on its proven low-noise performance, predictable costs and overall maturity of the architecture. The heritage for TDM is rooted in mm- and submm-wave experiments dating back 20 years and has since evolved to support a multiplexing factor of 64x in Stage-3 experiments.
author2 Département des Systèmes Basses Températures (DSBT )
Institut de Recherche Interdisciplinaire de Grenoble (IRIG)
Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA)
format Conference Object
author Schillaci, A.
Ade, P.A.R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Basu Thakur, R.
Bischoff, C.A.
Beck, D.
Bock, J.J.
Buza, V.
Cheshire, J.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A.
Denison, E.
Dierickx, M.
Duband, L.
Eiben, M.
Fatigoni, S.
Filippini, J.P.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D.
Grayson, J.A.
Grimes, P.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S.
Henderson, S.
Hildebrandt, S.R.
Hilton, G.C.
Hubmayr, J.
Hui, H.
Irwin, K.D.
Kang, J.
Karkare, K.S.
Kefeli, S.
Kovac, J.M.
Kuo, C.L.
Lau, K.
Leitch, E.M.
Lennox, A.
Megerian, K.G.
Miller, O.Y.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
author_facet Schillaci, A.
Ade, P.A.R.
Ahmed, Z.
Amiri, M.
Barkats, D.
Basu Thakur, R.
Bischoff, C.A.
Beck, D.
Bock, J.J.
Buza, V.
Cheshire, J.
Connors, J.
Cornelison, J.
Crumrine, M.
Cukierman, A.
Denison, E.
Dierickx, M.
Duband, L.
Eiben, M.
Fatigoni, S.
Filippini, J.P.
Giannakopoulos, C.
Goeckner-Wald, N.
Goldfinger, D.
Grayson, J.A.
Grimes, P.
Hall, G.
Halal, G.
Halpern, M.
Hand, E.
Harrison, S.
Henderson, S.
Hildebrandt, S.R.
Hilton, G.C.
Hubmayr, J.
Hui, H.
Irwin, K.D.
Kang, J.
Karkare, K.S.
Kefeli, S.
Kovac, J.M.
Kuo, C.L.
Lau, K.
Leitch, E.M.
Lennox, A.
Megerian, K.G.
Miller, O.Y.
Minutolo, L.
Moncelsi, L.
Nakato, Y.
author_sort Schillaci, A.
title BICEP Array: 150 GHz detector module development
title_short BICEP Array: 150 GHz detector module development
title_full BICEP Array: 150 GHz detector module development
title_fullStr BICEP Array: 150 GHz detector module development
title_full_unstemmed BICEP Array: 150 GHz detector module development
title_sort bicep array: 150 ghz detector module development
publisher HAL CCSD
publishDate 2021
url https://hal.science/hal-03483604
op_coverage Online Conference, United States
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source 19th International Workshop on Low Temperature Detectors
https://hal.science/hal-03483604
19th International Workshop on Low Temperature Detectors, Jul 2021, Online Conference, United States
op_relation info:eu-repo/semantics/altIdentifier/arxiv/2111.14785
hal-03483604
https://hal.science/hal-03483604
ARXIV: 2111.14785
INSPIRE: 1979391
_version_ 1766202924583616512