In-flight performance of SPIDER's 280 GHz receivers
International audience 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 N...
Published in: | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Conference Object |
Language: | English |
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2024
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Online Access: | https://hal.science/hal-04680943 https://doi.org/10.1117/12.3016837 |
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ftceafr:oai:HAL:hal-04680943v1 2024-09-30T14:26:56+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 Ericksen, 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 Luu, T.V Mason, P.V May, J Megerian, K Moncelsi, L Morford, T.A Nagy, J.M Nie, R Netterfield, C.B Nolta, M Osherson, B Padilla, I.L Rahlin, A.S Redmond, S Reintsema, C Romualdez, L.J Ruhl, J.E Runyan, M.C Shariff, J.A Shiu, C Soler, J.D Song, X Tartakovsky, S Thommesen, H Trangsrud, A Tucker, C Tucker, R.S Turner, A.D Ullom, J van der List, J.F van Lanen, J Vissers, M.R Weber, A.C Wen, S Wehus, I.K Wiebe, D.V Young, E.Y AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) Yokohama, Japan 2024-06-16 https://hal.science/hal-04680943 https://doi.org/10.1117/12.3016837 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2408.10444 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.3016837 hal-04680943 https://hal.science/hal-04680943 ARXIV: 2408.10444 doi:10.1117/12.3016837 INSPIRE: 2819788 Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2024 https://hal.science/hal-04680943 SPIE Astronomical Telescopes + Instrumentation 2024, Jun 2024, Yokohama, Japan. pp.1310204, ⟨10.1117/12.3016837⟩ [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2024 ftceafr https://doi.org/10.1117/12.3016837 2024-09-02T23:54:59Z International audience 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. Conference Object Antarc* Antarctic HAL-CEA (Commissariat à l'énergie atomique et aux énergies alternatives) Antarctic The Antarctic Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII 6 |
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Open Polar |
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HAL-CEA (Commissariat à l'énergie atomique et aux énergies alternatives) |
op_collection_id |
ftceafr |
language |
English |
topic |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] 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 Ericksen, 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 Luu, T.V Mason, P.V May, J Megerian, K Moncelsi, L Morford, T.A Nagy, J.M Nie, R Netterfield, C.B Nolta, M Osherson, B Padilla, I.L Rahlin, A.S Redmond, S Reintsema, C Romualdez, L.J Ruhl, J.E Runyan, M.C Shariff, J.A Shiu, C Soler, J.D Song, X Tartakovsky, S Thommesen, H Trangsrud, A Tucker, C Tucker, R.S Turner, A.D Ullom, J van der List, J.F van Lanen, J Vissers, M.R Weber, A.C Wen, S Wehus, I.K Wiebe, D.V Young, E.Y In-flight performance of SPIDER's 280 GHz receivers |
topic_facet |
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience 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. |
author2 |
AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) |
format |
Conference Object |
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 Ericksen, 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 Luu, T.V Mason, P.V May, J Megerian, K Moncelsi, L Morford, T.A Nagy, J.M Nie, R Netterfield, C.B Nolta, M Osherson, B Padilla, I.L Rahlin, A.S Redmond, S Reintsema, C Romualdez, L.J Ruhl, J.E Runyan, M.C Shariff, J.A Shiu, C Soler, J.D Song, X Tartakovsky, S Thommesen, H Trangsrud, A Tucker, C Tucker, R.S Turner, A.D Ullom, J van der List, J.F van Lanen, J Vissers, M.R Weber, A.C Wen, S Wehus, I.K Wiebe, D.V Young, E.Y |
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 Ericksen, 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 Luu, T.V Mason, P.V May, J Megerian, K Moncelsi, L Morford, T.A Nagy, J.M Nie, R Netterfield, C.B Nolta, M Osherson, B Padilla, I.L Rahlin, A.S Redmond, S Reintsema, C Romualdez, L.J Ruhl, J.E Runyan, M.C Shariff, J.A Shiu, C Soler, J.D Song, X Tartakovsky, S Thommesen, H Trangsrud, A Tucker, C Tucker, R.S Turner, A.D Ullom, J van der List, J.F van Lanen, J Vissers, M.R Weber, A.C Wen, S Wehus, I.K Wiebe, D.V Young, E.Y |
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 |
HAL CCSD |
publishDate |
2024 |
url |
https://hal.science/hal-04680943 https://doi.org/10.1117/12.3016837 |
op_coverage |
Yokohama, Japan |
geographic |
Antarctic The Antarctic |
geographic_facet |
Antarctic The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2024 https://hal.science/hal-04680943 SPIE Astronomical Telescopes + Instrumentation 2024, Jun 2024, Yokohama, Japan. pp.1310204, ⟨10.1117/12.3016837⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2408.10444 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.3016837 hal-04680943 https://hal.science/hal-04680943 ARXIV: 2408.10444 doi:10.1117/12.3016837 INSPIRE: 2819788 |
op_doi |
https://doi.org/10.1117/12.3016837 |
container_title |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII |
container_start_page |
6 |
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1811633067912069120 |