In-Flight Performance of Spider's 280 GHz Receivers ...
SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Ballo...
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Online Access: | https://dx.doi.org/10.48550/arxiv.2408.10444 https://arxiv.org/abs/2408.10444 |
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ftdatacite:10.48550/arxiv.2408.10444 2024-09-15T17:44:06+00:00 In-Flight Performance of Spider's 280 GHz Receivers ... Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. 2024 https://dx.doi.org/10.48550/arxiv.2408.10444 https://arxiv.org/abs/2408.10444 unknown arXiv Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 Instrumentation and Methods for Astrophysics astro-ph.IM Cosmology and Nongalactic Astrophysics astro-ph.CO FOS: Physical sciences CreativeWork Preprint Article article 2024 ftdatacite https://doi.org/10.48550/arxiv.2408.10444 2024-09-02T08:59:19Z SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Balloon flights above the Antarctic continent. During its first flight in January 2015, SPIDER observed in the 95 GHz and 150 GHz frequency bands, setting constraints on the B-mode signature of primordial gravitational waves. Its second flight in the 2022-23 season added new receivers at 280 GHz, each using an array of TESs coupled to the sky through feedhorns formed from stacks of silicon wafers. These receivers are optimized to produce deep maps of polarized Galactic dust emission over a large sky area, providing a unique data set with lasting value to the field. In this work, we describe the instrument's performance during SPIDER's second flight. ... : Submitted to SPIE Astronomical Telescopes + Instrumentation 2024, JATIS ... Article in Journal/Newspaper Antarc* Antarctic DataCite |
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Instrumentation and Methods for Astrophysics astro-ph.IM Cosmology and Nongalactic Astrophysics astro-ph.CO FOS: Physical sciences |
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Instrumentation and Methods for Astrophysics astro-ph.IM Cosmology and Nongalactic Astrophysics astro-ph.CO FOS: Physical sciences Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. In-Flight Performance of Spider's 280 GHz Receivers ... |
topic_facet |
Instrumentation and Methods for Astrophysics astro-ph.IM Cosmology and Nongalactic Astrophysics astro-ph.CO FOS: Physical sciences |
description |
SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Balloon flights above the Antarctic continent. During its first flight in January 2015, SPIDER observed in the 95 GHz and 150 GHz frequency bands, setting constraints on the B-mode signature of primordial gravitational waves. Its second flight in the 2022-23 season added new receivers at 280 GHz, each using an array of TESs coupled to the sky through feedhorns formed from stacks of silicon wafers. These receivers are optimized to produce deep maps of polarized Galactic dust emission over a large sky area, providing a unique data set with lasting value to the field. In this work, we describe the instrument's performance during SPIDER's second flight. ... : Submitted to SPIE Astronomical Telescopes + Instrumentation 2024, JATIS ... |
format |
Article in Journal/Newspaper |
author |
Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. |
author_facet |
Shaw, Elle C. Ade, P. A. R. Akers, S. Amiri, M. Austermann, J. Beall, J. Becker, D. T. Benton, S. J. Bergman, A. S. Bock, J. J. Bond, J. R. Bryan, S. A. Chiang, H. C. Contaldi, C. R. Domagalski, R. S. Doré, O. Duff, S. M. Duivenvoorden, A. J. Eriksen, H. K. Farhang, M. Filippini, J. P. Fissel, L. M. Fraisse, A. A. Freese, K. Galloway, M. Gambrel, A. E. Gandilo, N. N. Ganga, K. Gibbs, S. M. Gourapura, S. Grigorian, A. Gualtieri, R. Gudmundsson, J. E. Halpern, M. Hartley, J. Hasselfield, M. Hilton, G. Holmes, W. Hristov, V. V. Huang, Z. Hubmayr, J. Irwin, K. D. Jones, W. C. Kahn, A. Kermish, Z. D. King, C. Kuo, C. L. Lennox, A. R. Leung, J. S. -Y. Li, S. |
author_sort |
Shaw, Elle C. |
title |
In-Flight Performance of Spider's 280 GHz Receivers ... |
title_short |
In-Flight Performance of Spider's 280 GHz Receivers ... |
title_full |
In-Flight Performance of Spider's 280 GHz Receivers ... |
title_fullStr |
In-Flight Performance of Spider's 280 GHz Receivers ... |
title_full_unstemmed |
In-Flight Performance of Spider's 280 GHz Receivers ... |
title_sort |
in-flight performance of spider's 280 ghz receivers ... |
publisher |
arXiv |
publishDate |
2024 |
url |
https://dx.doi.org/10.48550/arxiv.2408.10444 https://arxiv.org/abs/2408.10444 |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_rights |
Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 |
op_doi |
https://doi.org/10.48550/arxiv.2408.10444 |
_version_ |
1810491454856888320 |