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

被引：0
|
作者：
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
机构：
[1] University of Illinois at Urbana-Champaign,Department of Physics
[2] University of Illinois at Urbana-Champaign,Department of Astronomy
[3] Cardiff University,School of Physics and Astronomy
[4] University of British Columbia,Department of Physics and Astronomy
[5] Princeton University,Department of Physics
[6] California Institute of Technology,Division of Physics, Mathematics and Astronomy
[7] Jet Propulsion Laboratory,Canadian Institute for Theoretical Astrophysics
[8] University of Toronto,School of Earth and Space Exploration
[9] Arizona State University,Department of Physics
[10] McGill University,Blackett Laboratory
[11] Imperial College London,Kavli Institute for Cosmological Physics
[12] University of Chicago,Department of Astronomy and Astrophysics
[13] University of Toronto,Department of Physics, The Oskar Klein Centre for Cosmoparticle Physics
[14] Stockholm University,Department of Physics
[15] AlbaNova,Department of Astronomy and Astrophysics
[16] University of Toronto,Department of Physics
[17] Pennsylvania State University,Physics Department
[18] National Institute of Standards and Technology,Department of Physics and Astronomy
[19] Stanford University,undefined
[20] SLAC National Accelerator Laboratory,undefined
[21] Case Western Reserve University,undefined
[22] Dunlap Institute for Astronomy,undefined
[23] Johns Hopkins University,undefined
[24] Fermi National Accelerator Laboratory,undefined
[25] Max-Planck-Institute for Astronomy,undefined
[26] Kavli Institute for Particle Astrophysics and Cosmology,undefined
来源：
Journal of Low Temperature Physics | 2020年 / 199卷
关键词：
Cosmic microwave background; Transition-edge sensor; Bolometer; Cosmic ray;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
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.
引用
收藏
页码：1127 / 1136
页数：9
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