Thermal testing for cryogenic CMB instrument optical design

D. C. Goldfinger; P. A.R. Ade; Z. Ahmed; M. Amiri; D. Barkats; R. Basu Thakur; D. Beck; C. A. Bischoff; J. J. Bock; V. Buza; James R Cheshire; J. Connors; J. Cornelison; Mike Crumrine; A. J. Cukierman; E. V. Denison; M. I. Dierickx; L. Duband; M. Eiben; S. Fatigoni; J. P. Filippini; C. Giannakopoulos; N. Goeckner-Wald; J. Grayson; P. K. Grimes; G. Hall; G. Halal; M. Halpern; E. Hand; S. A. Harrison; S. Henderson; S. R. Hildebrandt; G. C. Hilton; J. Hubmayr; H. Hui; K. D. Irwin; J. Kang; K. S. Karkare; S. Kefeli; J. M. Kovac; C. L. Kuo; Kenny Lau; E. M. Leitch; A. Lennox; T. Liu; K. G. Megerian; L. Minutolo; L. Moncelsi; Y. Nakato; T. Namikawa; H. T. Nguyen; R. O'Brient; S. Palladino; M. A. Petroff; T. Prouve; C. Pryke; B. Racine; C. D. Reintsema; M. Salatino; A. Schillaci; B. L. Schmitt; B. Singari; A. Soliman; A. G. Smith; T. St. Germaine; B. Steinbach; R. V. Sudiwala; K. L. Thompson; C. Tsai; C. Tucker; A. D. Turner; C. Umilta; C. Vergès; A. G. Vieregg; A. Wandui; A. C. Weber; D. V. Wiebe; Justin B Willmert; W. L.K. Wu; H. Yang; K. W. Yoon; E. Young; C. Yu; L. Zeng; C. Zhang; S. Zhang

doi:10.1117/12.2629490

Thermal testing for cryogenic CMB instrument optical design

D. C. Goldfinger
, P. A.R. Ade
, Z. Ahmed
, M. Amiri
, D. Barkats
, R. Basu Thakur
, D. Beck
, C. A. Bischoff
, J. J. Bock
, V. Buza
, James R Cheshire
, J. Connors
, J. Cornelison
, Mike Crumrine
, A. J. Cukierman
, E. V. Denison
, M. I. Dierickx
, L. Duband
, M. Eiben
, S. Fatigoni

J. P. Filippini, C. Giannakopoulos, N. Goeckner-Wald, J. Grayson, P. K. Grimes, G. Hall, G. Halal, M. Halpern, E. Hand, S. A. Harrison, S. Henderson, S. R. Hildebrandt, G. C. Hilton, J. Hubmayr, H. Hui, K. D. Irwin, J. Kang, K. S. Karkare, S. Kefeli, J. M. Kovac, C. L. Kuo, Kenny Lau, E. M. Leitch, A. Lennox, T. Liu, K. G. Megerian, L. Minutolo, L. Moncelsi, Y. Nakato, T. Namikawa, H. T. Nguyen, R. O'Brient, S. Palladino, M. A. Petroff, T. Prouve, C. Pryke, B. Racine, C. D. Reintsema, M. Salatino, A. Schillaci, B. L. Schmitt, B. Singari, A. Soliman, A. G. Smith, T. St. Germaine, B. Steinbach, R. V. Sudiwala, K. L. Thompson, C. Tsai, C. Tucker, A. D. Turner, C. Umilta, C. Vergès, A. G. Vieregg, A. Wandui, A. C. Weber, D. V. Wiebe, Justin B Willmert, W. L.K. Wu, H. Yang, K. W. Yoon, E. Young, C. Yu, L. Zeng, C. Zhang, S. Zhang

Physics and Astronomy (Twin Cities)

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

3 Scopus citations

Abstract

Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is therefore critical to optimize all aspects of the cryogenic design to achieve the necessary performance, with low temperature components and acceptable system cooling requirements. In particular, we will focus on our use of thermal filters and cold optics, which reduce the thermal load passed along to the cryogenic stages. To test their performance, we have made a series of in situ measurements while integrating the third receiver for the BICEP Array telescope. In addition to characterizing the behavior of this receiver, these measurements continue to refine the models that are being used to inform design choices being made for future instruments.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Electronic)	9781510653610
DOIs	https://doi.org/10.1117/12.2629490
State	Published - 2022
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022 - Montreal, Canada Duration: Jul 17 2022 → Jul 22 2022

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	12190
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022
Country/Territory	Canada
City	Montreal
Period	7/17/22 → 7/22/22

Bibliographical note

Funding Information:
The BICEP/Keck project (including BICEP2, BICEP3, and BICEP Array) have been made possible through a series of grants from the National Science Foundation including 0742818, 0742592, 1044978, 1110087, 1145172, 1145143, 1145248, 1639040, 1638957, 1638978, 1638970, 1726917, 1313010, 1313062, 1313158, 1313287, 0960243, 1836010, 1056465, & 1255358 and by the Keck Foundation. The development of antenna-coupled detector technology was supported by the JPL Research and Technology Development Fund and NASA Grants 06-ARPA206-0040, 10-SAT10-0017, 12-SAT12-0031, 14-SAT14-0009, 16-SAT16-0002, & 18-SAT18-0017. The development and testing of focal planes were supported by the Gordon and Betty Moore Foundation at Caltech. Readout electronics were supported by a Canada Foundation for Innovation grant to UBC. The computations in this paper were run on the Odyssey cluster supported by the FAS Science Division Research Computing Group at Harvard University. The analysis effort at Stanford and SLAC was partially supported by the Department of Energy, Contract DE-AC02-76SF00515. We thank the staff of the U.S. Antarctic Program and in particular the South Pole Station without whose help this research would not have been possible. Tireless administrative support was provided by Kathy Deniston, Sheri Stoll, Irene Coyle, Amy Dierker, Donna Hernandez, and Julie Shih.

Publisher Copyright:
© 2022 SPIE.

Keywords

BICEP Array
Cosmic Microwave Background
cryogenics
instrumentation
polarization
thermal Testing

Publisher link

10.1117/12.2629490

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Goldfinger, D. C., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Beck, D., Bischoff, C. A., Bock, J. J., Buza, V., Cheshire, J. R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A. J., Denison, E. V., Dierickx, M. I., Duband, L., Eiben, M., ... Zhang, S. (2022). Thermal testing for cryogenic CMB instrument optical design. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI Article 121901V (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12190). SPIE. https://doi.org/10.1117/12.2629490

Thermal testing for cryogenic CMB instrument optical design. / Goldfinger, D. C.; Ade, P. A.R.; Ahmed, Z. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2022. 121901V (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 12190).

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

Goldfinger, DC, Ade, PAR, Ahmed, Z, Amiri, M, Barkats, D, Basu Thakur, R, Beck, D, Bischoff, CA, Bock, JJ, Buza, V, Cheshire, JR, Connors, J, Cornelison, J, Crumrine, M, Cukierman, AJ, Denison, EV, Dierickx, MI, Duband, L, Eiben, M, Fatigoni, S, Filippini, JP, Giannakopoulos, C, Goeckner-Wald, N, Grayson, J, Grimes, PK, Hall, G, Halal, G, Halpern, M, Hand, E, Harrison, SA, Henderson, S, Hildebrandt, SR, Hilton, GC, Hubmayr, J, Hui, H, Irwin, KD, Kang, J, Karkare, KS, Kefeli, S, Kovac, JM, Kuo, CL, Lau, K, Leitch, EM, Lennox, A, Liu, T, Megerian, KG, Minutolo, L, Moncelsi, L, Nakato, Y, Namikawa, T, Nguyen, HT, O'Brient, R, Palladino, S, Petroff, MA, Prouve, T, Pryke, C, Racine, B, Reintsema, CD, Salatino, M, Schillaci, A, Schmitt, BL, Singari, B, Soliman, A, Smith, AG, St. Germaine, T, Steinbach, B, Sudiwala, RV, Thompson, KL, Tsai, C, Tucker, C, Turner, AD, Umilta, C, Vergès, C, Vieregg, AG, Wandui, A, Weber, AC, Wiebe, DV, Willmert, JB, Wu, WLK, Yang, H, Yoon, KW, Young, E, Yu, C, Zeng, L, Zhang, C & Zhang, S 2022, Thermal testing for cryogenic CMB instrument optical design. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI., 121901V, Proceedings of SPIE - The International Society for Optical Engineering, vol. 12190, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022, Montreal, Canada, 7/17/22. https://doi.org/10.1117/12.2629490

Goldfinger DC, Ade PAR, Ahmed Z, Amiri M, Barkats D, Basu Thakur R et al. Thermal testing for cryogenic CMB instrument optical design. In Zmuidzinas J, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI. SPIE. 2022. 121901V. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2629490

@inproceedings{87c0903a29aa47b681af736894da9bf2,

title = "Thermal testing for cryogenic CMB instrument optical design",

abstract = "Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is therefore critical to optimize all aspects of the cryogenic design to achieve the necessary performance, with low temperature components and acceptable system cooling requirements. In particular, we will focus on our use of thermal filters and cold optics, which reduce the thermal load passed along to the cryogenic stages. To test their performance, we have made a series of in situ measurements while integrating the third receiver for the BICEP Array telescope. In addition to characterizing the behavior of this receiver, these measurements continue to refine the models that are being used to inform design choices being made for future instruments.",

keywords = "BICEP Array, Cosmic Microwave Background, cryogenics, instrumentation, polarization, thermal Testing",

author = "Goldfinger, \{D. C.\} and Ade, \{P. A.R.\} and Z. Ahmed and M. Amiri and D. Barkats and \{Basu Thakur\}, R. and D. Beck and Bischoff, \{C. A.\} and Bock, \{J. J.\} and V. Buza and Cheshire, \{James R\} and J. Connors and J. Cornelison and Mike Crumrine and Cukierman, \{A. J.\} and Denison, \{E. V.\} and Dierickx, \{M. I.\} and L. Duband and M. Eiben and S. Fatigoni and Filippini, \{J. P.\} and C. Giannakopoulos and N. Goeckner-Wald and J. Grayson and Grimes, \{P. K.\} and G. Hall and G. Halal and M. Halpern and E. Hand and Harrison, \{S. A.\} and S. Henderson and Hildebrandt, \{S. R.\} and Hilton, \{G. C.\} and J. Hubmayr and H. Hui and Irwin, \{K. D.\} and J. Kang and Karkare, \{K. S.\} and S. Kefeli and Kovac, \{J. M.\} and Kuo, \{C. L.\} and Kenny Lau and Leitch, \{E. M.\} and A. Lennox and T. Liu and Megerian, \{K. G.\} and L. Minutolo and L. Moncelsi and Y. Nakato and T. Namikawa and Nguyen, \{H. T.\} and R. O'Brient and S. Palladino and Petroff, \{M. A.\} and T. Prouve and C. Pryke and B. Racine and Reintsema, \{C. D.\} and M. Salatino and A. Schillaci and Schmitt, \{B. L.\} and B. Singari and A. Soliman and Smith, \{A. G.\} and \{St. Germaine\}, T. and B. Steinbach and Sudiwala, \{R. V.\} and Thompson, \{K. L.\} and C. Tsai and C. Tucker and Turner, \{A. D.\} and C. Umilta and C. Verg{\`e}s and Vieregg, \{A. G.\} and A. Wandui and Weber, \{A. C.\} and Wiebe, \{D. V.\} and Willmert, \{Justin B\} and Wu, \{W. L.K.\} and H. Yang and Yoon, \{K. W.\} and E. Young and C. Yu and L. Zeng and C. Zhang and S. Zhang",

note = "Funding Information: The BICEP/Keck project (including BICEP2, BICEP3, and BICEP Array) have been made possible through a series of grants from the National Science Foundation including 0742818, 0742592, 1044978, 1110087, 1145172, 1145143, 1145248, 1639040, 1638957, 1638978, 1638970, 1726917, 1313010, 1313062, 1313158, 1313287, 0960243, 1836010, 1056465, \& 1255358 and by the Keck Foundation. The development of antenna-coupled detector technology was supported by the JPL Research and Technology Development Fund and NASA Grants 06-ARPA206-0040, 10-SAT10-0017, 12-SAT12-0031, 14-SAT14-0009, 16-SAT16-0002, \& 18-SAT18-0017. The development and testing of focal planes were supported by the Gordon and Betty Moore Foundation at Caltech. Readout electronics were supported by a Canada Foundation for Innovation grant to UBC. The computations in this paper were run on the Odyssey cluster supported by the FAS Science Division Research Computing Group at Harvard University. The analysis effort at Stanford and SLAC was partially supported by the Department of Energy, Contract DE-AC02-76SF00515. We thank the staff of the U.S. Antarctic Program and in particular the South Pole Station without whose help this research would not have been possible. Tireless administrative support was provided by Kathy Deniston, Sheri Stoll, Irene Coyle, Amy Dierker, Donna Hernandez, and Julie Shih. Publisher Copyright: {\textcopyright} 2022 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022 ; Conference date: 17-07-2022 Through 22-07-2022",

year = "2022",

doi = "10.1117/12.2629490",

language = "English (US)",

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

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao",

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

address = "United States",

}

TY - GEN

T1 - Thermal testing for cryogenic CMB instrument optical design

AU - Goldfinger, D. C.

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Amiri, M.

AU - Barkats, D.

AU - Basu Thakur, R.

AU - Beck, D.

AU - Bischoff, C. A.

AU - Bock, J. J.

AU - Buza, V.

AU - Cheshire, James R

AU - Connors, J.

AU - Cornelison, J.

AU - Crumrine, Mike

AU - Cukierman, A. J.

AU - Denison, E. V.

AU - Dierickx, M. I.

AU - Duband, L.

AU - Eiben, M.

AU - Fatigoni, S.

AU - Filippini, J. P.

AU - Giannakopoulos, C.

AU - Goeckner-Wald, N.

AU - Grayson, J.

AU - Grimes, P. K.

AU - Hall, G.

AU - Halal, G.

AU - Halpern, M.

AU - Hand, E.

AU - Harrison, S. A.

AU - Henderson, S.

AU - Hildebrandt, S. R.

AU - Hilton, G. C.

AU - Hubmayr, J.

AU - Hui, H.

AU - Irwin, K. D.

AU - Kang, J.

AU - Karkare, K. S.

AU - Kefeli, S.

AU - Kovac, J. M.

AU - Kuo, C. L.

AU - Lau, Kenny

AU - Leitch, E. M.

AU - Lennox, A.

AU - Liu, T.

AU - Megerian, K. G.

AU - Minutolo, L.

AU - Moncelsi, L.

AU - Nakato, Y.

AU - Namikawa, T.

AU - Nguyen, H. T.

AU - O'Brient, R.

AU - Palladino, S.

AU - Petroff, M. A.

AU - Prouve, T.

AU - Pryke, C.

AU - Racine, B.

AU - Reintsema, C. D.

AU - Salatino, M.

AU - Schillaci, A.

AU - Schmitt, B. L.

AU - Singari, B.

AU - Soliman, A.

AU - Smith, A. G.

AU - St. Germaine, T.

AU - Steinbach, B.

AU - Sudiwala, R. V.

AU - Thompson, K. L.

AU - Tsai, C.

AU - Tucker, C.

AU - Turner, A. D.

AU - Umilta, C.

AU - Vergès, C.

AU - Vieregg, A. G.

AU - Wandui, A.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Willmert, Justin B

AU - Wu, W. L.K.

AU - Yang, H.

AU - Yoon, K. W.

AU - Young, E.

AU - Yu, C.

AU - Zeng, L.

AU - Zhang, C.

AU - Zhang, S.

N1 - Funding Information: The BICEP/Keck project (including BICEP2, BICEP3, and BICEP Array) have been made possible through a series of grants from the National Science Foundation including 0742818, 0742592, 1044978, 1110087, 1145172, 1145143, 1145248, 1639040, 1638957, 1638978, 1638970, 1726917, 1313010, 1313062, 1313158, 1313287, 0960243, 1836010, 1056465, & 1255358 and by the Keck Foundation. The development of antenna-coupled detector technology was supported by the JPL Research and Technology Development Fund and NASA Grants 06-ARPA206-0040, 10-SAT10-0017, 12-SAT12-0031, 14-SAT14-0009, 16-SAT16-0002, & 18-SAT18-0017. The development and testing of focal planes were supported by the Gordon and Betty Moore Foundation at Caltech. Readout electronics were supported by a Canada Foundation for Innovation grant to UBC. The computations in this paper were run on the Odyssey cluster supported by the FAS Science Division Research Computing Group at Harvard University. The analysis effort at Stanford and SLAC was partially supported by the Department of Energy, Contract DE-AC02-76SF00515. We thank the staff of the U.S. Antarctic Program and in particular the South Pole Station without whose help this research would not have been possible. Tireless administrative support was provided by Kathy Deniston, Sheri Stoll, Irene Coyle, Amy Dierker, Donna Hernandez, and Julie Shih. Publisher Copyright: © 2022 SPIE.

PY - 2022

Y1 - 2022

N2 - Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is therefore critical to optimize all aspects of the cryogenic design to achieve the necessary performance, with low temperature components and acceptable system cooling requirements. In particular, we will focus on our use of thermal filters and cold optics, which reduce the thermal load passed along to the cryogenic stages. To test their performance, we have made a series of in situ measurements while integrating the third receiver for the BICEP Array telescope. In addition to characterizing the behavior of this receiver, these measurements continue to refine the models that are being used to inform design choices being made for future instruments.

AB - Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is therefore critical to optimize all aspects of the cryogenic design to achieve the necessary performance, with low temperature components and acceptable system cooling requirements. In particular, we will focus on our use of thermal filters and cold optics, which reduce the thermal load passed along to the cryogenic stages. To test their performance, we have made a series of in situ measurements while integrating the third receiver for the BICEP Array telescope. In addition to characterizing the behavior of this receiver, these measurements continue to refine the models that are being used to inform design choices being made for future instruments.

KW - BICEP Array

KW - Cosmic Microwave Background

KW - cryogenics

KW - instrumentation

KW - polarization

KW - thermal Testing

UR - https://www.scopus.com/pages/publications/85140730067

UR - https://www.scopus.com/pages/publications/85140730067#tab=citedBy

U2 - 10.1117/12.2629490

DO - 10.1117/12.2629490

M3 - Conference contribution

AN - SCOPUS:85140730067

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

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

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022

Y2 - 17 July 2022 through 22 July 2022

ER -

Thermal testing for cryogenic CMB instrument optical design

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