Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

Yaqiong Li; Kam Arnold; Zachary Atkins; Sarah Marie Bruno; Nicholas F. Cothard; Bradley Dober; Cody J. Duell; Shannon M. Duff; Patricio A. Gallardo; Erin Healy; Shuay Pwu Patty Ho; Johannes Hubmayr; Brian Keating; Adrian T. Lee; Aashrita Mangu; Heather McCarrick; Michael D. Niemack; Laura Newburgh; Christopher Raum; Maria Salatino; Trevor Sasse; Maximiliano Silva-Feaver; Sara M. Simon; Suzanne Staggs; Aritoki Suzuki; Joel Ullom; Eve M. Vavagiakis; Michael R. Vissers; Yuhan Wang; Benjamin Westbrook; Edward J. Wollack; Zhilei Xu; Kaiwen Zheng; Ningfeng Zhu

doi:10.1007/s10909-020-02386-6

Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

Yaqiong Li, Kam Arnold, Zachary Atkins, Sarah Marie Bruno, Nicholas F. Cothard, Bradley Dober, Cody J. Duell, Shannon M. Duff, Patricio A. Gallardo, Erin Healy, Shuay Pwu Patty Ho, Johannes Hubmayr, Brian Keating, Adrian T. Lee, Aashrita Mangu, Heather McCarrick, Michael D. Niemack, Laura Newburgh, Christopher Raum, Maria SalatinoTrevor Sasse, Maximiliano Silva-Feaver, Sara M. Simon, Suzanne Staggs, Aritoki Suzuki, Joel Ullom, Eve M. Vavagiakis, Michael R. Vissers, Yuhan Wang, Benjamin Westbrook, Edward J. Wollack, Zhilei Xu, Kaiwen Zheng, Ningfeng Zhu

Research output: Contribution to journal › Article › peer-review

7 Scopus citations

Abstract

The Simons Observatory will measure the cosmic microwave background temperature and polarization using a suite of new telescopes in the Atacama Desert in Chile.The Simons Observatory will use dichroic transition edge sensor (TES) bolometer arrays spanning six frequency bands from 27 to 280 GHz.The Simons Observatory will pioneer the use of a densely packed multiplexing architecture based on the microwave SQUID multiplexer (μmux), housing ∼2000 microwave resonators, each coupled to a TES. The Simons Observatory aims to multiplex each array of ∼2000 detectors with a single pair of coaxial cables and requires a multiplexing factor of ∼1000. The Simons Observatory cryogenic readout system is called the universal microwave multiplexing module (UMM). The UMM couples to both horn and lenslet-coupled detector arrays and is integrated into the universal focal-plane module (UFM) after being independently characterized. We present processes we have developed for highly repeatable and automated integration methods of UMMs, which will be needed for the production of the 49 UFMs required for the first stage of the Simons Observatory.

Original language	English (US)
Pages (from-to)	985-993
Number of pages	9
Journal	Journal of Low Temperature Physics
Volume	199
Issue number	3-4
DOIs	https://doi.org/10.1007/s10909-020-02386-6
State	Published - May 1 2020

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
General Materials Science
Condensed Matter Physics

Keywords

CMB
Multiplexing
Packaging
RF-SQUID
Readout
TES bolometers

Access to Document

10.1007/s10909-020-02386-6

Cite this

Li, Y., Arnold, K., Atkins, Z., Bruno, S. M., Cothard, N. F., Dober, B., Duell, C. J., Duff, S. M., Gallardo, P. A., Healy, E., Ho, S. P. P., Hubmayr, J., Keating, B., Lee, A. T., Mangu, A., McCarrick, H., Niemack, M. D., Newburgh, L., Raum, C., ... Zhu, N. (2020). Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory. Journal of Low Temperature Physics, 199(3-4), 985-993. https://doi.org/10.1007/s10909-020-02386-6

@article{8191a5e6853d4fae8a250d7f13787432,

title = "Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory",

abstract = "The Simons Observatory will measure the cosmic microwave background temperature and polarization using a suite of new telescopes in the Atacama Desert in Chile.The Simons Observatory will use dichroic transition edge sensor (TES) bolometer arrays spanning six frequency bands from 27 to 280 GHz.The Simons Observatory will pioneer the use of a densely packed multiplexing architecture based on the microwave SQUID multiplexer (μmux), housing ∼2000 microwave resonators, each coupled to a TES. The Simons Observatory aims to multiplex each array of ∼2000 detectors with a single pair of coaxial cables and requires a multiplexing factor of ∼1000. The Simons Observatory cryogenic readout system is called the universal microwave multiplexing module (UMM). The UMM couples to both horn and lenslet-coupled detector arrays and is integrated into the universal focal-plane module (UFM) after being independently characterized. We present processes we have developed for highly repeatable and automated integration methods of UMMs, which will be needed for the production of the 49 UFMs required for the first stage of the Simons Observatory.",

keywords = "CMB, Multiplexing, Packaging, RF-SQUID, Readout, TES bolometers",

author = "Yaqiong Li and Kam Arnold and Zachary Atkins and Bruno, {Sarah Marie} and Cothard, {Nicholas F.} and Bradley Dober and Duell, {Cody J.} and Duff, {Shannon M.} and Gallardo, {Patricio A.} and Erin Healy and Ho, {Shuay Pwu Patty} and Johannes Hubmayr and Brian Keating and Lee, {Adrian T.} and Aashrita Mangu and Heather McCarrick and Niemack, {Michael D.} and Laura Newburgh and Christopher Raum and Maria Salatino and Trevor Sasse and Maximiliano Silva-Feaver and Simon, {Sara M.} and Suzanne Staggs and Aritoki Suzuki and Joel Ullom and Vavagiakis, {Eve M.} and Vissers, {Michael R.} and Yuhan Wang and Benjamin Westbrook and Wollack, {Edward J.} and Zhilei Xu and Kaiwen Zheng and Ningfeng Zhu",

note = "Publisher Copyright: {\textcopyright} 2020, Springer Science+Business Media, LLC, part of Springer Nature.",

year = "2020",

month = may,

day = "1",

doi = "10.1007/s10909-020-02386-6",

language = "English (US)",

volume = "199",

pages = "985--993",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "3-4",

}

Li, Y, Arnold, K, Atkins, Z, Bruno, SM, Cothard, NF, Dober, B, Duell, CJ, Duff, SM, Gallardo, PA, Healy, E, Ho, SPP, Hubmayr, J, Keating, B, Lee, AT, Mangu, A, McCarrick, H, Niemack, MD, Newburgh, L, Raum, C, Salatino, M, Sasse, T, Silva-Feaver, M, Simon, SM, Staggs, S, Suzuki, A, Ullom, J, Vavagiakis, EM, Vissers, MR, Wang, Y, Westbrook, B, Wollack, EJ, Xu, Z, Zheng, K & Zhu, N 2020, 'Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory', Journal of Low Temperature Physics, vol. 199, no. 3-4, pp. 985-993. https://doi.org/10.1007/s10909-020-02386-6

TY - JOUR

T1 - Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

AU - Li, Yaqiong

AU - Arnold, Kam

AU - Atkins, Zachary

AU - Bruno, Sarah Marie

AU - Cothard, Nicholas F.

AU - Dober, Bradley

AU - Duell, Cody J.

AU - Duff, Shannon M.

AU - Gallardo, Patricio A.

AU - Healy, Erin

AU - Ho, Shuay Pwu Patty

AU - Hubmayr, Johannes

AU - Keating, Brian

AU - Lee, Adrian T.

AU - Mangu, Aashrita

AU - McCarrick, Heather

AU - Niemack, Michael D.

AU - Newburgh, Laura

AU - Raum, Christopher

AU - Salatino, Maria

AU - Sasse, Trevor

AU - Silva-Feaver, Maximiliano

AU - Simon, Sara M.

AU - Staggs, Suzanne

AU - Suzuki, Aritoki

AU - Ullom, Joel

AU - Vavagiakis, Eve M.

AU - Vissers, Michael R.

AU - Wang, Yuhan

AU - Westbrook, Benjamin

AU - Wollack, Edward J.

AU - Xu, Zhilei

AU - Zheng, Kaiwen

AU - Zhu, Ningfeng

PY - 2020/5/1

Y1 - 2020/5/1

N2 - The Simons Observatory will measure the cosmic microwave background temperature and polarization using a suite of new telescopes in the Atacama Desert in Chile.The Simons Observatory will use dichroic transition edge sensor (TES) bolometer arrays spanning six frequency bands from 27 to 280 GHz.The Simons Observatory will pioneer the use of a densely packed multiplexing architecture based on the microwave SQUID multiplexer (μmux), housing ∼2000 microwave resonators, each coupled to a TES. The Simons Observatory aims to multiplex each array of ∼2000 detectors with a single pair of coaxial cables and requires a multiplexing factor of ∼1000. The Simons Observatory cryogenic readout system is called the universal microwave multiplexing module (UMM). The UMM couples to both horn and lenslet-coupled detector arrays and is integrated into the universal focal-plane module (UFM) after being independently characterized. We present processes we have developed for highly repeatable and automated integration methods of UMMs, which will be needed for the production of the 49 UFMs required for the first stage of the Simons Observatory.

AB - The Simons Observatory will measure the cosmic microwave background temperature and polarization using a suite of new telescopes in the Atacama Desert in Chile.The Simons Observatory will use dichroic transition edge sensor (TES) bolometer arrays spanning six frequency bands from 27 to 280 GHz.The Simons Observatory will pioneer the use of a densely packed multiplexing architecture based on the microwave SQUID multiplexer (μmux), housing ∼2000 microwave resonators, each coupled to a TES. The Simons Observatory aims to multiplex each array of ∼2000 detectors with a single pair of coaxial cables and requires a multiplexing factor of ∼1000. The Simons Observatory cryogenic readout system is called the universal microwave multiplexing module (UMM). The UMM couples to both horn and lenslet-coupled detector arrays and is integrated into the universal focal-plane module (UFM) after being independently characterized. We present processes we have developed for highly repeatable and automated integration methods of UMMs, which will be needed for the production of the 49 UFMs required for the first stage of the Simons Observatory.

KW - CMB

KW - Multiplexing

KW - Packaging

KW - RF-SQUID

KW - Readout

KW - TES bolometers

UR - http://www.scopus.com/inward/record.url?scp=85081914815&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85081914815&partnerID=8YFLogxK

U2 - 10.1007/s10909-020-02386-6

DO - 10.1007/s10909-020-02386-6

M3 - Article

AN - SCOPUS:85081914815

SN - 0022-2291

VL - 199

SP - 985

EP - 993

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 3-4

ER -

Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

Abstract

All Science Journal Classification (ASJC) codes

Keywords

Access to Document

Other files and links

Fingerprint

Cite this