BICEP Array cryostat and mount design

Michael Crumrine; P. A.R. Ade; Z. Ahmed; R. W. Aikin; K. D. Alexander; D. Barkats; S. J. Benton; C. A. Bischoff; J. J. Bock; R. Bowens-Rubin; J. A. Brevik; I. Buder; E. Bullock; V. Buza; J. Connors; J. Cornelison; B. P. Crill; M. Dierickx; L. Duband; C. Dvorkin; J. P. Filippini; S. Fliescher; J. A. Grayson; G. Hall; M. Halpern; S. A. Harrison; S. R. Hildebrandt; G. C. Hilton; H. Hui; K. D. Irwin; J. H. Kang; K. S. Karkare; E. Karpel; J. P. Kaufman; B. G. Keating; S. Kefeli; S. A. Kernasovskiy; J. M. Kovac; C. L. Kuo; N. A. Larsen; K. Lau; E. M. Leitch; M. V. Lueker; K. G. Megerian; L. Moncelsi; T. Namikawa; C. B. Netterfield; H. T. Nguyen; R. O'Brient; R. W. Ogburn; S. Palladino; C. Pryke; B. Racine; S. Richter; R. Schwarz; A. Schillaci; C. D. Sheehy; A. Soliman; T. St Germaine; Z. K. Staniszewski; B. Steinbach; R. V. Sudiwala; G. P. Teply; K. L. Thompson; J. E. Tolan; C. E. Tucker; A. D. Turner; C. Umiltà; A. G. Vieregg; A. Wandui; A. C. Weber; D. V. Wiebe; J. Willmert; C. L. Wong; W. L.K. Wu; E. Yang; K. W. Yoon; C. Zhang

doi:10.1117/12.2312829

BICEP Array cryostat and mount design

Michael Crumrine, P. A.R. Ade, Z. Ahmed, R. W. Aikin, K. D. Alexander, D. Barkats, S. J. Benton, C. A. Bischoff, J. J. Bock, R. Bowens-Rubin, J. A. Brevik, I. Buder, E. Bullock, V. Buza, J. Connors, J. Cornelison, B. P. Crill, M. Dierickx, L. Duband, C. DvorkinJ. P. Filippini, S. Fliescher, J. A. Grayson, G. Hall, M. Halpern, S. A. Harrison, S. R. Hildebrandt, G. C. Hilton, H. Hui, K. D. Irwin, J. H. Kang, K. S. Karkare, E. Karpel, J. P. Kaufman, B. G. Keating, S. Kefeli, S. A. Kernasovskiy, J. M. Kovac, C. L. Kuo, N. A. Larsen, K. Lau, E. M. Leitch, M. V. Lueker, K. G. Megerian, L. Moncelsi, T. Namikawa, C. B. Netterfield, H. T. Nguyen, R. O'Brient, R. W. Ogburn, S. Palladino, C. Pryke, B. Racine, S. Richter, R. Schwarz, A. Schillaci, C. D. Sheehy, A. Soliman, T. St Germaine, Z. K. Staniszewski, B. Steinbach, R. V. Sudiwala, G. P. Teply, K. L. Thompson, J. E. Tolan, C. E. Tucker, A. D. Turner, C. Umiltà, A. G. Vieregg, A. Wandui, A. C. Weber, D. V. Wiebe, J. Willmert, C. L. Wong, W. L.K. Wu, E. Yang, K. W. Yoon, C. Zhang

Physics and Astronomy (Twin Cities)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

7 Scopus citations

Abstract

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.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Print)	9781510619692
DOIs	https://doi.org/10.1117/12.2312829
State	Published - 2018
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 - Austin, United States Duration: Jun 12 2018 → Jun 15 2018

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10708
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018
Country/Territory	United States
City	Austin
Period	6/12/18 → 6/15/18

Bibliographical note

Publisher Copyright:
© 2018 SPIE.

Keywords

BICEP
BICEP Array
Cosmology
Gravitational Waves
Inflation
Keck Array
Polarization

Access

10.1117/12.2312829

https://authors.library.caltech.edu/92193/1/107082D.pdf

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Crumrine, M., 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., ... Zhang, C. (2018). BICEP Array cryostat and mount design. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX Article 107082D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708). SPIE. https://doi.org/10.1117/12.2312829

BICEP Array cryostat and mount design. / Crumrine, Michael; Ade, P. A.R.; Ahmed, Z. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2018. 107082D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Crumrine, M, Ade, PAR, Ahmed, Z, Aikin, RW, Alexander, KD, Barkats, D, Benton, SJ, Bischoff, CA, Bock, JJ, Bowens-Rubin, R, Brevik, JA, Buder, I, Bullock, E, Buza, V, Connors, J, Cornelison, J, Crill, BP, Dierickx, M, Duband, L, Dvorkin, C, Filippini, JP, Fliescher, S, Grayson, JA, Hall, G, Halpern, M, Harrison, SA, Hildebrandt, SR, Hilton, GC, Hui, H, Irwin, KD, Kang, JH, Karkare, KS, Karpel, E, Kaufman, JP, Keating, BG, Kefeli, S, Kernasovskiy, SA, Kovac, JM, Kuo, CL, Larsen, NA, Lau, K, Leitch, EM, Lueker, MV, Megerian, KG, Moncelsi, L, Namikawa, T, Netterfield, CB, Nguyen, HT, O'Brient, R, Ogburn, RW, Palladino, S, Pryke, C, Racine, B, Richter, S, Schwarz, R, Schillaci, A, Sheehy, CD, Soliman, A, St Germaine, T, Staniszewski, ZK, Steinbach, B, Sudiwala, RV, Teply, GP, Thompson, KL, Tolan, JE, Tucker, CE, Turner, AD, Umiltà, C, Vieregg, AG, Wandui, A, Weber, AC, Wiebe, DV, Willmert, J, Wong, CL, Wu, WLK, Yang, E, Yoon, KW & Zhang, C 2018, BICEP Array cryostat and mount design. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX., 107082D, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10708, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018, Austin, United States, 6/12/18. https://doi.org/10.1117/12.2312829

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abstract = "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.",

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note = "Publisher Copyright: {\textcopyright} 2018 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 ; Conference date: 12-06-2018 Through 15-06-2018",

year = "2018",

doi = "10.1117/12.2312829",

language = "English (US)",

isbn = "9781510619692",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

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booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX",

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TY - GEN

T1 - BICEP Array cryostat and mount design

AU - Crumrine, Michael

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Aikin, R. W.

AU - Alexander, K. D.

AU - Barkats, D.

AU - Benton, S. J.

AU - Bischoff, C. A.

AU - Bock, J. J.

AU - Bowens-Rubin, R.

AU - Brevik, J. A.

AU - Buder, I.

AU - Bullock, E.

AU - Buza, V.

AU - Connors, J.

AU - Cornelison, J.

AU - Crill, B. P.

AU - Dierickx, M.

AU - Duband, L.

AU - Dvorkin, C.

AU - Filippini, J. P.

AU - Fliescher, S.

AU - Grayson, J. A.

AU - Hall, G.

AU - Halpern, M.

AU - Harrison, S. A.

AU - Hildebrandt, S. R.

AU - Hilton, G. C.

AU - Hui, H.

AU - Irwin, K. D.

AU - Kang, J. H.

AU - Karkare, K. S.

AU - Karpel, E.

AU - Kaufman, J. P.

AU - Keating, B. G.

AU - Kefeli, S.

AU - Kernasovskiy, S. A.

AU - Kovac, J. M.

AU - Kuo, C. L.

AU - Larsen, N. A.

AU - Lau, K.

AU - Leitch, E. M.

AU - Lueker, M. V.

AU - Megerian, K. G.

AU - Moncelsi, L.

AU - Namikawa, T.

AU - Netterfield, C. B.

AU - Nguyen, H. T.

AU - O'Brient, R.

AU - Ogburn, R. W.

AU - Palladino, S.

AU - Pryke, C.

AU - Racine, B.

AU - Richter, S.

AU - Schwarz, R.

AU - Schillaci, A.

AU - Sheehy, C. D.

AU - Soliman, A.

AU - St Germaine, T.

AU - Staniszewski, Z. K.

AU - Steinbach, B.

AU - Sudiwala, R. V.

AU - Teply, G. P.

AU - Thompson, K. L.

AU - Tolan, J. E.

AU - Tucker, C. E.

AU - Turner, A. D.

AU - Umiltà, C.

AU - Vieregg, A. G.

AU - Wandui, A.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Willmert, J.

AU - Wong, C. L.

AU - Wu, W. L.K.

AU - Yang, E.

AU - Yoon, K. W.

AU - Zhang, C.

PY - 2018

Y1 - 2018

N2 - 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.

AB - 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.

KW - BICEP

KW - BICEP Array

KW - Cosmology

KW - Gravitational Waves

KW - Inflation

KW - Keck Array

KW - Polarization

UR - http://www.scopus.com/inward/record.url?scp=85051994905&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85051994905&partnerID=8YFLogxK

U2 - 10.1117/12.2312829

DO - 10.1117/12.2312829

M3 - Conference contribution

AN - SCOPUS:85051994905

SN - 9781510619692

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018

Y2 - 12 June 2018 through 15 June 2018

ER -

BICEP Array cryostat and mount design

Abstract

Publication series

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Bibliographical note

Keywords

Access

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