Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory

B. Osherson; J. P. Filippini; J. Fu; R. V. Gramillano; R. Gualtieri; E. C. Shaw; P. A.R. Ade; M. Amiri; S. J. Benton; J. J. Bock; J. R. Bond; S. A. Bryan; H. C. Chiang; C. R. Contaldi; O. Dore; A. A. Fraisse; A. E. Gambrel; N. N. Gandilo; J. E. Gudmundsson; M. Halpern; J. W. Hartley; M. Hasselfield; G. Hilton; W. Holmes; V. V. Hristov; K. D. Irwin; W. C. Jones; Z. D. Kermish; P. V. Mason; K. Megerian; L. Moncelsi; T. A. Morford; J. M. Nagy; C. B. Netterfield; I. L. Padilla; A. S. Rahlin; C. Reintsema; J. E. Ruhl; M. C. Runyan; J. A. Shariff; J. D. Soler; A. Trangsrud; C. Tucker; R. S. Tucker; A. D. Turner; A. C. Weber; D. V. Wiebe; E. Y. Young

doi:10.1007/s10909-020-02415-4

Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory

B. Osherson, J. P. Filippini, J. Fu, R. V. Gramillano, R. Gualtieri, E. C. Shaw, P. A.R. Ade, M. Amiri, S. J. Benton, J. J. Bock, J. R. Bond, S. A. Bryan, H. C. Chiang, C. R. Contaldi, O. Dore, A. A. Fraisse, A. E. Gambrel, N. N. Gandilo, J. E. Gudmundsson, M. HalpernJ. W. Hartley, M. Hasselfield, G. Hilton, W. Holmes, V. V. Hristov, K. D. Irwin, W. C. Jones, Z. D. Kermish, P. V. Mason, K. Megerian, L. Moncelsi, T. A. Morford, J. M. Nagy, C. B. Netterfield, I. L. Padilla, A. S. Rahlin, C. Reintsema, J. E. Ruhl, M. C. Runyan, J. A. Shariff, J. D. Soler, A. Trangsrud, C. Tucker, R. S. Tucker, A. D. Turner, A. C. Weber, D. V. Wiebe, E. Y. Young

Physics

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

3 Scopus citations

Abstract

Future mm-wave and sub-mm space missions will employ large arrays of multiplexed transition-edge-sensor (TES) bolometers. Such instruments must contend with the high flux of cosmic rays beyond our atmosphere that induce ‘glitches’ in bolometer data, which posed a challenge to data analysis from the Planck bolometers. Future instruments will face the additional challenges of shared substrate wafers and multiplexed readout wiring. In this work, we explore the susceptibility of modern TES arrays to the cosmic ray environment of space using two data sets: the 2015 long-duration balloon flight of the SPIDER cosmic microwave background polarimeter, and a laboratory exposure of SPIDER flight hardware to radioactive sources. We find manageable glitch rates and short glitch durations, leading to minimal effect on SPIDER analysis. We constrain energy propagation within the substrate through a study of multi-detector coincidences and give a preliminary look at pulse shapes in laboratory data.

Original language	English (US)
Pages (from-to)	1127-1136
Number of pages	10
Journal	Journal of Low Temperature Physics
Volume	199
Issue number	3-4
DOIs	https://doi.org/10.1007/s10909-020-02415-4
State	Published - May 1 2020

All Science Journal Classification (ASJC) codes

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

Keywords

Bolometer
Cosmic microwave background
Cosmic ray
Transition-edge sensor

Access to Document

10.1007/s10909-020-02415-4

Cite this

Osherson, B., Filippini, J. P., Fu, J., Gramillano, R. V., Gualtieri, R., Shaw, E. C., Ade, P. A. R., Amiri, M., Benton, S. J., Bock, J. J., Bond, J. R., Bryan, S. A., Chiang, H. C., Contaldi, C. R., Dore, O., Fraisse, A. A., Gambrel, A. E., Gandilo, N. N., Gudmundsson, J. E., ... Young, E. Y. (2020). Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory. Journal of Low Temperature Physics, 199(3-4), 1127-1136. https://doi.org/10.1007/s10909-020-02415-4

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title = "Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory",

abstract = "Future mm-wave and sub-mm space missions will employ large arrays of multiplexed transition-edge-sensor (TES) bolometers. Such instruments must contend with the high flux of cosmic rays beyond our atmosphere that induce {\textquoteleft}glitches{\textquoteright} in bolometer data, which posed a challenge to data analysis from the Planck bolometers. Future instruments will face the additional challenges of shared substrate wafers and multiplexed readout wiring. In this work, we explore the susceptibility of modern TES arrays to the cosmic ray environment of space using two data sets: the 2015 long-duration balloon flight of the SPIDER cosmic microwave background polarimeter, and a laboratory exposure of SPIDER flight hardware to radioactive sources. We find manageable glitch rates and short glitch durations, leading to minimal effect on SPIDER analysis. We constrain energy propagation within the substrate through a study of multi-detector coincidences and give a preliminary look at pulse shapes in laboratory data.",

keywords = "Bolometer, Cosmic microwave background, Cosmic ray, Transition-edge sensor",

author = "B. Osherson and Filippini, {J. P.} and J. Fu and Gramillano, {R. V.} and R. Gualtieri and Shaw, {E. C.} and Ade, {P. A.R.} and M. Amiri and Benton, {S. J.} and Bock, {J. J.} and Bond, {J. R.} and Bryan, {S. A.} and Chiang, {H. C.} and Contaldi, {C. R.} and O. Dore and Fraisse, {A. A.} and Gambrel, {A. E.} and Gandilo, {N. N.} and Gudmundsson, {J. E.} and M. Halpern and Hartley, {J. W.} and M. Hasselfield and G. Hilton and W. Holmes and Hristov, {V. V.} and Irwin, {K. D.} and Jones, {W. C.} and Kermish, {Z. D.} and Mason, {P. V.} and K. Megerian and L. Moncelsi and Morford, {T. A.} and Nagy, {J. M.} and Netterfield, {C. B.} and Padilla, {I. L.} and Rahlin, {A. S.} and C. Reintsema and Ruhl, {J. E.} and Runyan, {M. C.} and Shariff, {J. A.} and Soler, {J. D.} and A. Trangsrud and C. Tucker and Tucker, {R. S.} and Turner, {A. D.} and Weber, {A. C.} and Wiebe, {D. V.} and Young, {E. Y.}",

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

year = "2020",

month = may,

day = "1",

doi = "10.1007/s10909-020-02415-4",

language = "English (US)",

volume = "199",

pages = "1127--1136",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "3-4",

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Osherson, B, Filippini, JP, Fu, J, Gramillano, RV, Gualtieri, R, Shaw, EC, Ade, PAR, Amiri, M, Benton, SJ, Bock, JJ, Bond, JR, Bryan, SA, Chiang, HC, Contaldi, CR, Dore, O, Fraisse, AA, Gambrel, AE, Gandilo, NN, Gudmundsson, JE, Halpern, M, Hartley, JW, Hasselfield, M, Hilton, G, Holmes, W, Hristov, VV, Irwin, KD, Jones, WC, Kermish, ZD, Mason, PV, Megerian, K, Moncelsi, L, Morford, TA, Nagy, JM, Netterfield, CB, Padilla, IL, Rahlin, AS, Reintsema, C, Ruhl, JE, Runyan, MC, Shariff, JA, Soler, JD, Trangsrud, A, Tucker, C, Tucker, RS, Turner, AD, Weber, AC, Wiebe, DV & Young, EY 2020, 'Particle Response of Antenna-Coupled TES Arrays: Results from SPIDER and the Laboratory', Journal of Low Temperature Physics, vol. 199, no. 3-4, pp. 1127-1136. https://doi.org/10.1007/s10909-020-02415-4

TY - JOUR

T1 - Particle Response of Antenna-Coupled TES Arrays

T2 - Results from SPIDER and the Laboratory

AU - Osherson, B.

AU - Filippini, J. P.

AU - Fu, J.

AU - Gramillano, R. V.

AU - Gualtieri, R.

AU - Shaw, E. C.

AU - Ade, P. A.R.

AU - Amiri, M.

AU - Benton, S. J.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Bryan, S. A.

AU - Chiang, H. C.

AU - Contaldi, C. R.

AU - Dore, O.

AU - Fraisse, A. A.

AU - Gambrel, A. E.

AU - Gandilo, N. N.

AU - Gudmundsson, J. E.

AU - Halpern, M.

AU - Hartley, J. W.

AU - Hasselfield, M.

AU - Hilton, G.

AU - Holmes, W.

AU - Hristov, V. V.

AU - Irwin, K. D.

AU - Jones, W. C.

AU - Kermish, Z. D.

AU - Mason, P. V.

AU - Megerian, K.

AU - Moncelsi, L.

AU - Morford, T. A.

AU - Nagy, J. M.

AU - Netterfield, C. B.

AU - Padilla, I. L.

AU - Rahlin, A. S.

AU - Reintsema, C.

AU - Ruhl, J. E.

AU - Runyan, M. C.

AU - Shariff, J. A.

AU - Soler, J. D.

AU - Trangsrud, A.

AU - Tucker, C.

AU - Tucker, R. S.

AU - Turner, A. D.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Young, E. Y.

PY - 2020/5/1

Y1 - 2020/5/1

N2 - Future mm-wave and sub-mm space missions will employ large arrays of multiplexed transition-edge-sensor (TES) bolometers. Such instruments must contend with the high flux of cosmic rays beyond our atmosphere that induce ‘glitches’ in bolometer data, which posed a challenge to data analysis from the Planck bolometers. Future instruments will face the additional challenges of shared substrate wafers and multiplexed readout wiring. In this work, we explore the susceptibility of modern TES arrays to the cosmic ray environment of space using two data sets: the 2015 long-duration balloon flight of the SPIDER cosmic microwave background polarimeter, and a laboratory exposure of SPIDER flight hardware to radioactive sources. We find manageable glitch rates and short glitch durations, leading to minimal effect on SPIDER analysis. We constrain energy propagation within the substrate through a study of multi-detector coincidences and give a preliminary look at pulse shapes in laboratory data.

AB - Future mm-wave and sub-mm space missions will employ large arrays of multiplexed transition-edge-sensor (TES) bolometers. Such instruments must contend with the high flux of cosmic rays beyond our atmosphere that induce ‘glitches’ in bolometer data, which posed a challenge to data analysis from the Planck bolometers. Future instruments will face the additional challenges of shared substrate wafers and multiplexed readout wiring. In this work, we explore the susceptibility of modern TES arrays to the cosmic ray environment of space using two data sets: the 2015 long-duration balloon flight of the SPIDER cosmic microwave background polarimeter, and a laboratory exposure of SPIDER flight hardware to radioactive sources. We find manageable glitch rates and short glitch durations, leading to minimal effect on SPIDER analysis. We constrain energy propagation within the substrate through a study of multi-detector coincidences and give a preliminary look at pulse shapes in laboratory data.

KW - Bolometer

KW - Cosmic microwave background

KW - Cosmic ray

KW - Transition-edge sensor

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UR - http://www.scopus.com/inward/citedby.url?scp=85082195636&partnerID=8YFLogxK

U2 - 10.1007/s10909-020-02415-4

DO - 10.1007/s10909-020-02415-4

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SN - 0022-2291

VL - 199

SP - 1127

EP - 1136

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

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