In Situ Performance of the Low Frequency Array for Advanced ACTPol

Yaqiong Li; Jason E. Austermann; James A. Beall; Sarah Marie Bruno; Steve K. Choi; Nicholas F. Cothard; Kevin T. Crowley; Shannon M. Duff; Shuay Pwu Patty Ho; Joseph E. Golec; Gene C. Hilton; Matthew Hasselfield; Johannes Hubmayr; Brian J. Koopman; Marius Lungu; Jeff McMahon; Michael D. Niemack; Lyman A. Page; Maria Salatino; Sara M. Simon; Suzanne T. Staggs; Jason R. Stevens; Joel N. Ullom; Eve M. Vavagiakis; Yuhan Wang; Edward J. Wollack; Zhilei Xu

doi:10.1109/TASC.2021.3063334

In Situ Performance of the Low Frequency Array for Advanced ACTPol

Yaqiong Li, Jason E. Austermann, James A. Beall, Sarah Marie Bruno, Steve K. Choi, Nicholas F. Cothard, Kevin T. Crowley, Shannon M. Duff, Shuay Pwu Patty Ho, Joseph E. Golec, Gene C. Hilton, Matthew Hasselfield, Johannes Hubmayr, Brian J. Koopman, Marius Lungu, Jeff McMahon, Michael D. Niemack, Lyman A. Page, Maria Salatino, Sara M. SimonSuzanne T. Staggs, Jason R. Stevens, Joel N. Ullom, Eve M. Vavagiakis, Yuhan Wang, Edward J. Wollack, Zhilei Xu

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5 Scopus citations

Abstract

The AdvancedAtacama Cosmology Telescope Polarimeter (AdvACT) [1] is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies. The low frequency (LF) array was deployed early 2020. It consists of 292 TES bolometers observing in two bands centered at 27 GHz and 39 GHz. At these frequencies, it is sensitive to synchrotron radiation from our galaxy as well as to the CMB, and complements the AdvACT arrays operating at 90, 150 and 230 GHz. We present the initial LF array on-site characterization, including the time constant, optical efficiency and array sensitivity.

Original language	English (US)
Article number	9369015
Journal	IEEE Transactions on Applied Superconductivity
Volume	31
Issue number	5
DOIs	https://doi.org/10.1109/TASC.2021.3063334
State	Published - Aug 2021

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Electrical and Electronic Engineering

Keywords

Superconducting detectors
transition edge sensor

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10.1109/TASC.2021.3063334

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Li, Y., Austermann, J. E., Beall, J. A., Bruno, S. M., Choi, S. K., Cothard, N. F., Crowley, K. T., Duff, S. M., Ho, S. P. P., Golec, J. E., Hilton, G. C., Hasselfield, M., Hubmayr, J., Koopman, B. J., Lungu, M., McMahon, J., Niemack, M. D., Page, L. A., Salatino, M., ... Xu, Z. (2021). In Situ Performance of the Low Frequency Array for Advanced ACTPol. IEEE Transactions on Applied Superconductivity, 31(5), Article 9369015. https://doi.org/10.1109/TASC.2021.3063334

@article{5fdaa65e4ba84085a675cd36b5f4b1e1,

title = "In Situ Performance of the Low Frequency Array for Advanced ACTPol",

abstract = "The AdvancedAtacama Cosmology Telescope Polarimeter (AdvACT) [1] is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies. The low frequency (LF) array was deployed early 2020. It consists of 292 TES bolometers observing in two bands centered at 27 GHz and 39 GHz. At these frequencies, it is sensitive to synchrotron radiation from our galaxy as well as to the CMB, and complements the AdvACT arrays operating at 90, 150 and 230 GHz. We present the initial LF array on-site characterization, including the time constant, optical efficiency and array sensitivity.",

keywords = "Superconducting detectors, transition edge sensor",

author = "Yaqiong Li and Austermann, {Jason E.} and Beall, {James A.} and Bruno, {Sarah Marie} and Choi, {Steve K.} and Cothard, {Nicholas F.} and Crowley, {Kevin T.} and Duff, {Shannon M.} and Ho, {Shuay Pwu Patty} and Golec, {Joseph E.} and Hilton, {Gene C.} and Matthew Hasselfield and Johannes Hubmayr and Koopman, {Brian J.} and Marius Lungu and Jeff McMahon and Niemack, {Michael D.} and Page, {Lyman A.} and Maria Salatino and Simon, {Sara M.} and Staggs, {Suzanne T.} and Stevens, {Jason R.} and Ullom, {Joel N.} and Vavagiakis, {Eve M.} and Yuhan Wang and Wollack, {Edward J.} and Zhilei Xu",

note = "Publisher Copyright: {\textcopyright} 2002-2011 IEEE.",

year = "2021",

month = aug,

doi = "10.1109/TASC.2021.3063334",

language = "English (US)",

volume = "31",

journal = "IEEE Transactions on Applied Superconductivity",

issn = "1051-8223",

publisher = "Institute of Electrical and Electronics Engineers Inc.",

number = "5",

}

Li, Y, Austermann, JE, Beall, JA, Bruno, SM, Choi, SK, Cothard, NF, Crowley, KT, Duff, SM, Ho, SPP, Golec, JE, Hilton, GC, Hasselfield, M, Hubmayr, J, Koopman, BJ, Lungu, M, McMahon, J, Niemack, MD, Page, LA, Salatino, M, Simon, SM, Staggs, ST, Stevens, JR, Ullom, JN, Vavagiakis, EM, Wang, Y, Wollack, EJ & Xu, Z 2021, 'In Situ Performance of the Low Frequency Array for Advanced ACTPol', IEEE Transactions on Applied Superconductivity, vol. 31, no. 5, 9369015. https://doi.org/10.1109/TASC.2021.3063334

TY - JOUR

T1 - In Situ Performance of the Low Frequency Array for Advanced ACTPol

AU - Li, Yaqiong

AU - Austermann, Jason E.

AU - Beall, James A.

AU - Bruno, Sarah Marie

AU - Choi, Steve K.

AU - Cothard, Nicholas F.

AU - Crowley, Kevin T.

AU - Duff, Shannon M.

AU - Ho, Shuay Pwu Patty

AU - Golec, Joseph E.

AU - Hilton, Gene C.

AU - Hasselfield, Matthew

AU - Hubmayr, Johannes

AU - Koopman, Brian J.

AU - Lungu, Marius

AU - McMahon, Jeff

AU - Niemack, Michael D.

AU - Page, Lyman A.

AU - Salatino, Maria

AU - Simon, Sara M.

AU - Staggs, Suzanne T.

AU - Stevens, Jason R.

AU - Ullom, Joel N.

AU - Vavagiakis, Eve M.

AU - Wang, Yuhan

AU - Wollack, Edward J.

AU - Xu, Zhilei

PY - 2021/8

Y1 - 2021/8

N2 - The AdvancedAtacama Cosmology Telescope Polarimeter (AdvACT) [1] is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies. The low frequency (LF) array was deployed early 2020. It consists of 292 TES bolometers observing in two bands centered at 27 GHz and 39 GHz. At these frequencies, it is sensitive to synchrotron radiation from our galaxy as well as to the CMB, and complements the AdvACT arrays operating at 90, 150 and 230 GHz. We present the initial LF array on-site characterization, including the time constant, optical efficiency and array sensitivity.

AB - The AdvancedAtacama Cosmology Telescope Polarimeter (AdvACT) [1] is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarization anisotropies in multiple frequencies. The low frequency (LF) array was deployed early 2020. It consists of 292 TES bolometers observing in two bands centered at 27 GHz and 39 GHz. At these frequencies, it is sensitive to synchrotron radiation from our galaxy as well as to the CMB, and complements the AdvACT arrays operating at 90, 150 and 230 GHz. We present the initial LF array on-site characterization, including the time constant, optical efficiency and array sensitivity.

KW - Superconducting detectors

KW - transition edge sensor

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U2 - 10.1109/TASC.2021.3063334

DO - 10.1109/TASC.2021.3063334

M3 - Article

AN - SCOPUS:85102290516

SN - 1051-8223

VL - 31

JO - IEEE Transactions on Applied Superconductivity

JF - IEEE Transactions on Applied Superconductivity

IS - 5

M1 - 9369015

ER -

In Situ Performance of the Low Frequency Array for Advanced ACTPol

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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