Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays

Kevin T. Crowley; Jason E. Austermann; Steve K. Choi; Shannon M. Duff; Patricio A. Gallardo; Shuay Pwu Patty Ho; Johannes Hubmayr; Brian J. Koopman; Federico Nati; Michael D. Niemack; Maria Salatino; Sara M. Simon; Suzanne T. Staggs; Jason R. Stevens; Joel N. Ullom; Eve M. Vavagiakis; Edward J. Wollack

doi:10.1007/s10909-018-2028-7

Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays

Kevin T. Crowley, Jason E. Austermann, Steve K. Choi, Shannon M. Duff, Patricio A. Gallardo, Shuay Pwu Patty Ho, Johannes Hubmayr, Brian J. Koopman, Federico Nati, Michael D. Niemack, Maria Salatino, Sara M. Simon, Suzanne T. Staggs, Jason R. Stevens, Joel N. Ullom, Eve M. Vavagiakis, Edward J. Wollack

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

12 Scopus citations

Abstract

The Advanced ACTPol (AdvACT) upgrade to the Atacama Cosmology Telescope (ACT) features arrays of aluminum manganese transition-edge sensors (TESes) optimized for ground-based observations of the cosmic microwave background (CMB). Array testing shows highly responsive detectors with anticipated in-band noise performance under optical loading. We report on TES parameters measured with impedance data taken on a subset of TESes. We then compare modeled noise spectral densities to measurements. We find excess noise at frequencies around 100 Hz, nearly outside of the signal band of CMB measurements. In addition, we describe full-array noise measurements in the laboratory and in the field for two new AdvACT mid-frequency arrays, sensitive at bands centered on 90 and 150 GHz, and data for the high-frequency array (150/230 GHz) as deployed.

Original language	English (US)
Pages (from-to)	328-336
Number of pages	9
Journal	Journal of Low Temperature Physics
Volume	193
Issue number	3-4
DOIs	https://doi.org/10.1007/s10909-018-2028-7
State	Published - Nov 1 2018

All Science Journal Classification (ASJC) codes

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

Keywords

Cosmic microwave background
Detector modeling
Noise performance
TES parameters
Transition-edge sensor

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10.1007/s10909-018-2028-7

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Crowley, K. T., Austermann, J. E., Choi, S. K., Duff, S. M., Gallardo, P. A., Ho, S. P. P., Hubmayr, J., Koopman, B. J., Nati, F., Niemack, M. D., Salatino, M., Simon, S. M., Staggs, S. T., Stevens, J. R., Ullom, J. N., Vavagiakis, E. M., & Wollack, E. J. (2018). Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays. Journal of Low Temperature Physics, 193(3-4), 328-336. https://doi.org/10.1007/s10909-018-2028-7

@article{2ed827d2b5cb47c583f04a78de334ce4,

title = "Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays",

abstract = "The Advanced ACTPol (AdvACT) upgrade to the Atacama Cosmology Telescope (ACT) features arrays of aluminum manganese transition-edge sensors (TESes) optimized for ground-based observations of the cosmic microwave background (CMB). Array testing shows highly responsive detectors with anticipated in-band noise performance under optical loading. We report on TES parameters measured with impedance data taken on a subset of TESes. We then compare modeled noise spectral densities to measurements. We find excess noise at frequencies around 100 Hz, nearly outside of the signal band of CMB measurements. In addition, we describe full-array noise measurements in the laboratory and in the field for two new AdvACT mid-frequency arrays, sensitive at bands centered on 90 and 150 GHz, and data for the high-frequency array (150/230 GHz) as deployed.",

keywords = "Cosmic microwave background, Detector modeling, Noise performance, TES parameters, Transition-edge sensor",

author = "Crowley, {Kevin T.} and Austermann, {Jason E.} and Choi, {Steve K.} and Duff, {Shannon M.} and Gallardo, {Patricio A.} and Ho, {Shuay Pwu Patty} and Johannes Hubmayr and Koopman, {Brian J.} and Federico Nati and Niemack, {Michael D.} and Maria Salatino and Simon, {Sara M.} and Staggs, {Suzanne T.} and Stevens, {Jason R.} and Ullom, {Joel N.} and Vavagiakis, {Eve M.} and Wollack, {Edward J.}",

note = "Publisher Copyright: {\textcopyright} 2018, Springer Science+Business Media, LLC, part of Springer Nature.",

year = "2018",

month = nov,

day = "1",

doi = "10.1007/s10909-018-2028-7",

language = "English (US)",

volume = "193",

pages = "328--336",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "3-4",

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Crowley, KT, Austermann, JE, Choi, SK, Duff, SM, Gallardo, PA, Ho, SPP, Hubmayr, J, Koopman, BJ, Nati, F, Niemack, MD, Salatino, M, Simon, SM, Staggs, ST, Stevens, JR, Ullom, JN, Vavagiakis, EM & Wollack, EJ 2018, 'Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays', Journal of Low Temperature Physics, vol. 193, no. 3-4, pp. 328-336. https://doi.org/10.1007/s10909-018-2028-7

TY - JOUR

T1 - Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays

AU - Crowley, Kevin T.

AU - Austermann, Jason E.

AU - Choi, Steve K.

AU - Duff, Shannon M.

AU - Gallardo, Patricio A.

AU - Ho, Shuay Pwu Patty

AU - Hubmayr, Johannes

AU - Koopman, Brian J.

AU - Nati, Federico

AU - Niemack, Michael D.

AU - Salatino, Maria

AU - Simon, Sara M.

AU - Staggs, Suzanne T.

AU - Stevens, Jason R.

AU - Ullom, Joel N.

AU - Vavagiakis, Eve M.

AU - Wollack, Edward J.

PY - 2018/11/1

Y1 - 2018/11/1

N2 - The Advanced ACTPol (AdvACT) upgrade to the Atacama Cosmology Telescope (ACT) features arrays of aluminum manganese transition-edge sensors (TESes) optimized for ground-based observations of the cosmic microwave background (CMB). Array testing shows highly responsive detectors with anticipated in-band noise performance under optical loading. We report on TES parameters measured with impedance data taken on a subset of TESes. We then compare modeled noise spectral densities to measurements. We find excess noise at frequencies around 100 Hz, nearly outside of the signal band of CMB measurements. In addition, we describe full-array noise measurements in the laboratory and in the field for two new AdvACT mid-frequency arrays, sensitive at bands centered on 90 and 150 GHz, and data for the high-frequency array (150/230 GHz) as deployed.

AB - The Advanced ACTPol (AdvACT) upgrade to the Atacama Cosmology Telescope (ACT) features arrays of aluminum manganese transition-edge sensors (TESes) optimized for ground-based observations of the cosmic microwave background (CMB). Array testing shows highly responsive detectors with anticipated in-band noise performance under optical loading. We report on TES parameters measured with impedance data taken on a subset of TESes. We then compare modeled noise spectral densities to measurements. We find excess noise at frequencies around 100 Hz, nearly outside of the signal band of CMB measurements. In addition, we describe full-array noise measurements in the laboratory and in the field for two new AdvACT mid-frequency arrays, sensitive at bands centered on 90 and 150 GHz, and data for the high-frequency array (150/230 GHz) as deployed.

KW - Cosmic microwave background

KW - Detector modeling

KW - Noise performance

KW - TES parameters

KW - Transition-edge sensor

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DO - 10.1007/s10909-018-2028-7

M3 - Article

AN - SCOPUS:85051104580

SN - 0022-2291

VL - 193

SP - 328

EP - 336

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 3-4

ER -

Advanced ACTPol TES Device Parameters and Noise Performance in Fielded Arrays

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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