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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04189naa a2200925 4500 | |
| 001 | oai:DiVA.org:su-183144 | |
| 003 | SwePub | |
| 008 | 200702s2020 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1831442 URI |
| 024 | 7 | a https://doi.org/10.1007/s10909-020-02415-42 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Osherson, B.4 aut |
| 245 | 1 0 | a Particle Response of Antenna-Coupled TES Arrays :b Results from SPIDER and the Laboratory |
| 264 | c 2020-03-13 | |
| 264 | 1 | b Springer Science and Business Media LLC,c 2020 |
| 338 | a print2 rdacarrier | |
| 520 | a 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. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Cosmic microwave background | |
| 653 | a Transition-edge sensor | |
| 653 | a Bolometer | |
| 653 | a Cosmic ray | |
| 700 | 1 | a Filippini, J. P.4 aut |
| 700 | 1 | a Fu, J.4 aut |
| 700 | 1 | a Gramillano, R.4 aut |
| 700 | 1 | a Gualtieri, R.4 aut |
| 700 | 1 | a Shaw, E. C.4 aut |
| 700 | 1 | a Ade, P. A. R.4 aut |
| 700 | 1 | a Amiri, M.4 aut |
| 700 | 1 | a Benton, S. J.4 aut |
| 700 | 1 | a Bock, J. J.4 aut |
| 700 | 1 | a Bond, J. R.4 aut |
| 700 | 1 | a Bryan, S. A.4 aut |
| 700 | 1 | a Chiang, H. C.4 aut |
| 700 | 1 | a Contaldi, C. R.4 aut |
| 700 | 1 | a Dore, O.4 aut |
| 700 | 1 | a Fraisse, A. A.4 aut |
| 700 | 1 | a Gambrel, A. E.4 aut |
| 700 | 1 | a Gandilo, N. N.4 aut |
| 700 | 1 | a Gudmundsson, Jón E.u Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jgudm |
| 700 | 1 | a Halpern, M.4 aut |
| 700 | 1 | a Hartley, J. W.4 aut |
| 700 | 1 | a Hasselfield, M.4 aut |
| 700 | 1 | a Hilton, G.4 aut |
| 700 | 1 | a Holmes, W.4 aut |
| 700 | 1 | a Hristov, V. V.4 aut |
| 700 | 1 | a Irwin, K. D.4 aut |
| 700 | 1 | a Jones, W. C.4 aut |
| 700 | 1 | a Kermish, Z. D.4 aut |
| 700 | 1 | a Mason, P.4 aut |
| 700 | 1 | a Megerian, K.4 aut |
| 700 | 1 | a Moncelsi, L.4 aut |
| 700 | 1 | a Morford, T. A.4 aut |
| 700 | 1 | a Nagy, J. M.4 aut |
| 700 | 1 | a Netterfield, C. B.4 aut |
| 700 | 1 | a Padilla, I. L.4 aut |
| 700 | 1 | a Rahlin, A. S.4 aut |
| 700 | 1 | a Reintsema, C.4 aut |
| 700 | 1 | a Ruhl, J. E.4 aut |
| 700 | 1 | a Runyan, M. C.4 aut |
| 700 | 1 | a Shariff, J. A.4 aut |
| 700 | 1 | a Soler, J. D.4 aut |
| 700 | 1 | a Trangsrud, A.4 aut |
| 700 | 1 | a Tucker, C.4 aut |
| 700 | 1 | a Tucker, R. S.4 aut |
| 700 | 1 | a Turner, A. D.4 aut |
| 700 | 1 | a Weber, A. C.4 aut |
| 700 | 1 | a Wiebe, D.4 aut |
| 700 | 1 | a Young, E. Y.4 aut |
| 710 | 2 | a Stockholms universitetb Fysikum4 org |
| 773 | 0 | t Journal of Low Temperature Physicsd : Springer Science and Business Media LLCg 199:3-4, s. 1127-1136q 199:3-4<1127-1136x 0022-2291x 1573-7357 |
| 856 | 4 | u https://arxiv.org/abs/2002.05771y arXiv:2002.05771 |
| 856 | 4 | u https://authors.library.caltech.edu/101905/3/2002.05771.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-183144 |
| 856 | 4 8 | u https://doi.org/10.1007/s10909-020-02415-4 |
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