Imperial College London
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Carlo R. Contaldi

Faculty of Natural Sciences, Department of Physics

Professor of Theoretical Physics
 
 
 
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Contact

 

+44 (0)20 7594 1527c.contaldi

 
 
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Location

 

505Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Osherson:2020:10.1007/s10909-020-02415-4,
author = {Osherson, B and Filippini, JP and Fu, J and Gramillano, R and Gualtieri, R and Shaw, EC and Ade, PAR and Amiri, M and Benton, SJ and Bock, JJ and Bond, JR and Bryan, SA and Chiang, HC and Contaldi, CR and Dore, O and Fraisse, AA and Gambrel, AE and Gandilo, NN and Gudmundsson, JE and Halpern, M and Hartley, JW and Hasselfield, M and Hilton, G and Holmes, W and Hristov, VV and Irwin, KD and Jones, WC and Kermish, ZD and Mason, P and Megerian, K and Moncelsi, L and Morford, TA and Nagy, JM and Netterfield, CB and Padilla, IL and Rahlin, AS and Reintsema, C and Ruhl, JE and Runyan, MC and Shariff, JA and Soler, JD and Trangsrud, A and Tucker, C and Tucker, RS and Turner, AD and Weber, AC and Wiebe, D and Young, EY},
doi = {10.1007/s10909-020-02415-4},
journal = {Journal of Low Temperature Physics},
pages = {1127--1136},
title = {Particle response of antenna-coupled TES arrays: results from SPIDER and the laboratory},
url = {http://dx.doi.org/10.1007/s10909-020-02415-4},
volume = {199},
year = {2020}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
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.
AU  - Osherson,B
AU  - Filippini,JP
AU  - Fu,J
AU  - Gramillano,R
AU  - Gualtieri,R
AU  - Shaw,EC
AU  - Ade,PAR
AU  - Amiri,M
AU  - Benton,SJ
AU  - Bock,JJ
AU  - Bond,JR
AU  - Bryan,SA
AU  - Chiang,HC
AU  - Contaldi,CR
AU  - Dore,O
AU  - Fraisse,AA
AU  - Gambrel,AE
AU  - Gandilo,NN
AU  - Gudmundsson,JE
AU  - Halpern,M
AU  - Hartley,JW
AU  - Hasselfield,M
AU  - Hilton,G
AU  - Holmes,W
AU  - Hristov,VV
AU  - Irwin,KD
AU  - Jones,WC
AU  - Kermish,ZD
AU  - Mason,P
AU  - Megerian,K
AU  - Moncelsi,L
AU  - Morford,TA
AU  - Nagy,JM
AU  - Netterfield,CB
AU  - Padilla,IL
AU  - Rahlin,AS
AU  - Reintsema,C
AU  - Ruhl,JE
AU  - Runyan,MC
AU  - Shariff,JA
AU  - Soler,JD
AU  - Trangsrud,A
AU  - Tucker,C
AU  - Tucker,RS
AU  - Turner,AD
AU  - Weber,AC
AU  - Wiebe,D
AU  - Young,EY
DO  - 10.1007/s10909-020-02415-4
EP  - 1136
PY  - 2020///
SN  - 0022-2291
SP  - 1127
TI  - Particle response of antenna-coupled TES arrays: results from SPIDER and the laboratory
T2  - Journal of Low Temperature Physics
UR  - http://dx.doi.org/10.1007/s10909-020-02415-4
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000531902200067&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://link.springer.com/article/10.1007%2Fs10909-020-02415-4
UR  - http://hdl.handle.net/10044/1/81979
VL  - 199
ER  -
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