Design and pre-flight performance of SPIDER 280 GHz receivers

E. C. Shaw; P. A.R. Ade; S. Akers; M. Amiri; J. E. Austermann; J. A. Beall; D. T. Becker; S. J. Benton; A. S. Bergman; J. J. Bock; J. R. Bond; S. A. Bryan; H. C. Chiang; C. R. Contaldi; R. S. Domagalski; O. Dore; S. M. Duff; A. J. Duivenvoorden; H. K. Eriksen; M. Farhang; J. P. Filippini; L. M. Fissel; A. A. Fraisse; K. Freese; M. Galloway; A. E. Gambrel; N. N. Gandilo; K. Ganga; A. Grigorian; R. Gualtieri; J. E. Gudmundsson; M. Halpern; J. Hartley; M. Hasselfield; G. Hilton; W. Holmes; V. V. Hristov; Z. Huang; J. Hubmayr; K. D. Irwin; W. C. Jones; A. Kahn; C. L. Kuo; Z. D. Kermish; A. Lennox; J. S.Y. Leung; S. Li; P. V. Mason; K. Megerian; L. M. Mocanu; L. Moncelsi; T. A. Morford; J. M. Nagy; R. Nie; M. Nolta; C. B. Netterfield; B. Osherson; I. L. Padilla; A. S. Rahlin; S. Redmond; C. Reintsema; M. C. Runyan; L. J. Romualdez; J. E. Ruhl; J. A. Shariff; C. Shiu; J. D. Soler; X. Song; A. Trangsrud; H. Thommesen; C. Tucker; R. S. Tucker; A. D. Turner; J. Ullom; J. F. Van Der List; J. Van Lanen; M. R. Vissers; A. C. Weber; S. Wen; I. K. Wehus; D. V. Wiebe; E. Y. Young

doi:10.1117/12.2562941

Design and pre-flight performance of SPIDER 280 GHz receivers

E. C. Shaw, P. A.R. Ade, S. Akers, M. Amiri, J. E. Austermann, J. A. Beall, D. T. Becker, S. J. Benton, A. S. Bergman, J. J. Bock, J. R. Bond, S. A. Bryan, H. C. Chiang, C. R. Contaldi, R. S. Domagalski, O. Dore, S. M. Duff, A. J. Duivenvoorden, H. K. Eriksen, M. FarhangJ. P. Filippini, L. M. Fissel, A. A. Fraisse, K. Freese, M. Galloway, A. E. Gambrel, N. N. Gandilo, K. Ganga, A. Grigorian, R. Gualtieri, J. E. Gudmundsson, M. Halpern, J. Hartley, M. Hasselfield, G. Hilton, W. Holmes, V. V. Hristov, Z. Huang, J. Hubmayr, K. D. Irwin, W. C. Jones, A. Kahn, C. L. Kuo, Z. D. Kermish, A. Lennox, J. S.Y. Leung, S. Li, P. V. Mason, K. Megerian, L. M. Mocanu, L. Moncelsi, T. A. Morford, J. M. Nagy, R. Nie, M. Nolta, C. B. Netterfield, B. Osherson, I. L. Padilla, A. S. Rahlin, S. Redmond, C. Reintsema, M. C. Runyan, L. J. Romualdez, J. E. Ruhl, J. A. Shariff, C. Shiu, J. D. Soler, X. Song, A. Trangsrud, H. Thommesen, C. Tucker, R. S. Tucker, A. D. Turner, J. Ullom, J. F. Van Der List, J. Van Lanen, M. R. Vissers, A. C. Weber, S. Wen, I. K. Wehus, D. V. Wiebe, E. Y. Young

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

3 Scopus citations

Abstract

In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature in the cosmic microwave background at degree angular scales. During its first flight in 2015, Spider mapped ∼10% of the sky at 95 and 150 GHz. The payload for the second Antarctic flight will incorporate three new 280 GHz receivers alongside three refurbished 95-and 150 GHz receivers from Spider's first flight. In this work we discuss the design and characterization of these new receivers, which employ over 1500 feedhorn-coupled transition-edge sensors. We describe pre-flight laboratory measurements of detector properties, and the optical performance of completed receivers. These receivers will map a wide area of the sky at 280 GHz, providing new information on polarized Galactic dust emission that will help to separate it from the cosmological signal.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Electronic)	9781510636934
DOIs	https://doi.org/10.1117/12.2562941
State	Published - 2020
Externally published	Yes
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 - Virtual, Online, United States Duration: Dec 14 2020 → Dec 22 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11453
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020
Country/Territory	United States
City	Virtual, Online
Period	12/14/20 → 12/22/20

Keywords

Spider
cosmic microwave background
cosmology
millimeter wave instrumentation
polarization
scientific ballooning
scientific instrumentation
transition-edge sensor

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2562941

Cite this

Shaw, E. C., Ade, P. A. R., Akers, S., Amiri, M., Austermann, J. E., Beall, J. A., 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., Dore, O., Duff, S. M., Duivenvoorden, A. J., Eriksen, H. K., ... Young, E. Y. (2020). Design and pre-flight performance of SPIDER 280 GHz receivers. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X Article 114532F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453). SPIE. https://doi.org/10.1117/12.2562941

Design and pre-flight performance of SPIDER 280 GHz receivers. / Shaw, E. C.; Ade, P. A.R.; Akers, S. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2020. 114532F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Shaw, EC, Ade, PAR, Akers, S, Amiri, M, Austermann, JE, Beall, JA, Becker, DT, Benton, SJ, Bergman, AS, Bock, JJ, Bond, JR, Bryan, SA, Chiang, HC, Contaldi, CR, Domagalski, RS, Dore, O, Duff, SM, Duivenvoorden, AJ, Eriksen, HK, Farhang, M, Filippini, JP, Fissel, LM, Fraisse, AA, Freese, K, Galloway, M, Gambrel, AE, Gandilo, NN, Ganga, K, Grigorian, A, Gualtieri, R, Gudmundsson, JE, Halpern, M, Hartley, J, Hasselfield, M, Hilton, G, Holmes, W, Hristov, VV, Huang, Z, Hubmayr, J, Irwin, KD, Jones, WC, Kahn, A, Kuo, CL, Kermish, ZD, Lennox, A, Leung, JSY, Li, S, Mason, PV, Megerian, K, Mocanu, LM, Moncelsi, L, Morford, TA, Nagy, JM, Nie, R, Nolta, M, Netterfield, CB, Osherson, B, Padilla, IL, Rahlin, AS, Redmond, S, Reintsema, C, Runyan, MC, Romualdez, LJ, Ruhl, JE, Shariff, JA, Shiu, C, Soler, JD, Song, X, Trangsrud, A, Thommesen, H, Tucker, C, Tucker, RS, Turner, AD, Ullom, J, Van Der List, JF, Van Lanen, J, Vissers, MR, Weber, AC, Wen, S, Wehus, IK, Wiebe, DV & Young, EY 2020, Design and pre-flight performance of SPIDER 280 GHz receivers. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X., 114532F, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11453, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020, Virtual, Online, United States, 12/14/20. https://doi.org/10.1117/12.2562941

Shaw EC, Ade PAR, Akers S, Amiri M, Austermann JE, Beall JA et al. Design and pre-flight performance of SPIDER 280 GHz receivers. In Zmuidzinas J, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. SPIE. 2020. 114532F. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2562941

@inproceedings{018694590d9f4cf9a8b7f295548df97c,

title = "Design and pre-flight performance of SPIDER 280 GHz receivers",

abstract = "In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature in the cosmic microwave background at degree angular scales. During its first flight in 2015, Spider mapped ∼10% of the sky at 95 and 150 GHz. The payload for the second Antarctic flight will incorporate three new 280 GHz receivers alongside three refurbished 95-and 150 GHz receivers from Spider's first flight. In this work we discuss the design and characterization of these new receivers, which employ over 1500 feedhorn-coupled transition-edge sensors. We describe pre-flight laboratory measurements of detector properties, and the optical performance of completed receivers. These receivers will map a wide area of the sky at 280 GHz, providing new information on polarized Galactic dust emission that will help to separate it from the cosmological signal.",

keywords = "Spider, cosmic microwave background, cosmology, millimeter wave instrumentation, polarization, scientific ballooning, scientific instrumentation, transition-edge sensor",

author = "Shaw, {E. C.} and Ade, {P. A.R.} and S. Akers and M. Amiri and Austermann, {J. E.} and Beall, {J. A.} and Becker, {D. T.} and Benton, {S. J.} and Bergman, {A. S.} and Bock, {J. J.} and Bond, {J. R.} and Bryan, {S. A.} and Chiang, {H. C.} and Contaldi, {C. R.} and Domagalski, {R. S.} and O. Dore and Duff, {S. M.} and Duivenvoorden, {A. J.} and Eriksen, {H. K.} and M. Farhang and Filippini, {J. P.} and Fissel, {L. M.} and Fraisse, {A. A.} and K. Freese and M. Galloway and Gambrel, {A. E.} and Gandilo, {N. N.} and K. Ganga and A. Grigorian and R. Gualtieri and Gudmundsson, {J. E.} and M. Halpern and J. Hartley and M. Hasselfield and G. Hilton and W. Holmes and Hristov, {V. V.} and Z. Huang and J. Hubmayr and Irwin, {K. D.} and Jones, {W. C.} and A. Kahn and Kuo, {C. L.} and Kermish, {Z. D.} and A. Lennox and Leung, {J. S.Y.} and S. Li and Mason, {P. V.} and K. Megerian and Mocanu, {L. M.} and L. Moncelsi and Morford, {T. A.} and Nagy, {J. M.} and R. Nie and M. Nolta and Netterfield, {C. B.} and B. Osherson and Padilla, {I. L.} and Rahlin, {A. S.} and S. Redmond and C. Reintsema and Runyan, {M. C.} and Romualdez, {L. J.} and Ruhl, {J. E.} and Shariff, {J. A.} and C. Shiu and Soler, {J. D.} and X. Song and A. Trangsrud and H. Thommesen and C. Tucker and Tucker, {R. S.} and Turner, {A. D.} and J. Ullom and {Van Der List}, {J. F.} and {Van Lanen}, J. and Vissers, {M. R.} and Weber, {A. C.} and S. Wen and Wehus, {I. K.} and Wiebe, {D. V.} and Young, {E. Y.}",

note = "Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2562941",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao",

booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X",

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TY - GEN

T1 - Design and pre-flight performance of SPIDER 280 GHz receivers

AU - Shaw, E. C.

AU - Ade, P. A.R.

AU - Akers, S.

AU - Amiri, M.

AU - Austermann, J. E.

AU - Beall, J. A.

AU - Becker, D. T.

AU - Benton, S. J.

AU - Bergman, A. S.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Bryan, S. A.

AU - Chiang, H. C.

AU - Contaldi, C. R.

AU - Domagalski, R. S.

AU - Dore, O.

AU - Duff, S. M.

AU - Duivenvoorden, A. J.

AU - Eriksen, H. K.

AU - Farhang, M.

AU - Filippini, J. P.

AU - Fissel, L. M.

AU - Fraisse, A. A.

AU - Freese, K.

AU - Galloway, M.

AU - Gambrel, A. E.

AU - Gandilo, N. N.

AU - Ganga, K.

AU - Grigorian, A.

AU - Gualtieri, R.

AU - Gudmundsson, J. E.

AU - Halpern, M.

AU - Hartley, J.

AU - Hasselfield, M.

AU - Hilton, G.

AU - Holmes, W.

AU - Hristov, V. V.

AU - Huang, Z.

AU - Hubmayr, J.

AU - Irwin, K. D.

AU - Jones, W. C.

AU - Kahn, A.

AU - Kuo, C. L.

AU - Kermish, Z. D.

AU - Lennox, A.

AU - Leung, J. S.Y.

AU - Li, S.

AU - Mason, P. V.

AU - Megerian, K.

AU - Mocanu, L. M.

AU - Moncelsi, L.

AU - Morford, T. A.

AU - Nagy, J. M.

AU - Nie, R.

AU - Nolta, M.

AU - Netterfield, C. B.

AU - Osherson, B.

AU - Padilla, I. L.

AU - Rahlin, A. S.

AU - Redmond, S.

AU - Reintsema, C.

AU - Runyan, M. C.

AU - Romualdez, L. J.

AU - Ruhl, J. E.

AU - Shariff, J. A.

AU - Shiu, C.

AU - Soler, J. D.

AU - Song, X.

AU - Trangsrud, A.

AU - Thommesen, H.

AU - Tucker, C.

AU - Tucker, R. S.

AU - Turner, A. D.

AU - Ullom, J.

AU - Van Der List, J. F.

AU - Van Lanen, J.

AU - Vissers, M. R.

AU - Weber, A. C.

AU - Wen, S.

AU - Wehus, I. K.

AU - Wiebe, D. V.

AU - Young, E. Y.

PY - 2020

Y1 - 2020

N2 - In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature in the cosmic microwave background at degree angular scales. During its first flight in 2015, Spider mapped ∼10% of the sky at 95 and 150 GHz. The payload for the second Antarctic flight will incorporate three new 280 GHz receivers alongside three refurbished 95-and 150 GHz receivers from Spider's first flight. In this work we discuss the design and characterization of these new receivers, which employ over 1500 feedhorn-coupled transition-edge sensors. We describe pre-flight laboratory measurements of detector properties, and the optical performance of completed receivers. These receivers will map a wide area of the sky at 280 GHz, providing new information on polarized Galactic dust emission that will help to separate it from the cosmological signal.

AB - In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature in the cosmic microwave background at degree angular scales. During its first flight in 2015, Spider mapped ∼10% of the sky at 95 and 150 GHz. The payload for the second Antarctic flight will incorporate three new 280 GHz receivers alongside three refurbished 95-and 150 GHz receivers from Spider's first flight. In this work we discuss the design and characterization of these new receivers, which employ over 1500 feedhorn-coupled transition-edge sensors. We describe pre-flight laboratory measurements of detector properties, and the optical performance of completed receivers. These receivers will map a wide area of the sky at 280 GHz, providing new information on polarized Galactic dust emission that will help to separate it from the cosmological signal.

KW - Spider

KW - cosmic microwave background

KW - cosmology

KW - millimeter wave instrumentation

KW - polarization

KW - scientific ballooning

KW - scientific instrumentation

KW - transition-edge sensor

UR - http://www.scopus.com/inward/record.url?scp=85100062713&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85100062713&partnerID=8YFLogxK

U2 - 10.1117/12.2562941

DO - 10.1117/12.2562941

M3 - Conference contribution

AN - SCOPUS:85100062713

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020

Y2 - 14 December 2020 through 22 December 2020

ER -

Design and pre-flight performance of SPIDER 280 GHz receivers

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Keywords

ASJC Scopus subject areas

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