Pre-flight integration and characterization of the SPIDER balloon-borne telescope

A. S. Rahlin; P. A.R. Ade; M. Amiri; S. J. Benton; J. J. Bock; J. R. Bond; S. A. Bryan; Hsin C. Chiang; C. R. Contaldi; B. P. Crill; O. Doré; M. Farhang; J. P. Filippini; L. M. Fissel; A. A. Fraisse; A. E. Gambrel; N. N. Gandilo; S. Golwala; Jon E. Gudmundsson; M. Halpern; M. F. Hasselfield; G. Hilton; W. A. Holmes; V. V. Hristov; K. D. Irwin; William C. Jones; Zigmund D. Kermish; C. L. Kuo; C. J. MacTavish; P. V. Mason; K. Megerian; L. Moncelsi; T. A. Morford; J. M. Nagy; C. B. Netterfield; R. O'Brient; 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

doi:10.1117/12.2055683

Pre-flight integration and characterization of the SPIDER balloon-borne telescope

A. S. Rahlin
, P. A.R. Ade
, M. Amiri
, S. J. Benton
, J. J. Bock
, J. R. Bond
, S. A. Bryan
, Hsin C. Chiang
, C. R. Contaldi
, B. P. Crill
, O. Doré
, M. Farhang
, J. P. Filippini
, L. M. Fissel
, A. A. Fraisse
, A. E. Gambrel
, N. N. Gandilo
, S. Golwala
, Jon E. Gudmundsson
, M. Halpern

M. F. Hasselfield, G. Hilton, W. A. Holmes, V. V. Hristov, K. D. Irwin, William C. Jones, Zigmund D. Kermish, C. L. Kuo, C. J. MacTavish, P. V. Mason, K. Megerian, L. Moncelsi, T. A. Morford, J. M. Nagy, C. B. Netterfield, R. O'Brient, 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

Astronomy & Astrophysics

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

37 Scopus citations

Abstract

We present the results of integration and characterization of the Spider instrument after the 2013 pre-flight campaign. Spider is a balloon-borne polarimeter designed to probe the primordial gravitational wave signal in the degree-scale B-mode polarization of the cosmic microwave background. With six independent telescopes housing over 2000 detectors in the 94 GHz and 150 GHz frequency bands, Spider will map 7.5% of the sky with a depth of 11 to 14 μ 1/4K .arcmin at each frequency, which is a factor of ∼5 improvement over Planck. We discuss the integration of the pointing, cryogenic, electronics, and power sub-systems, as well as pre-flight characterization of the detectors and optical systems. Spider is well prepared for a December 2014 flight from Antarctica, and is expected to be limited by astrophysical foreground emission, and not instrumental sensitivity, over the survey region.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Editors	Jonas Zmuidzinas, Wayne S. Holland
Publisher	SPIE
ISBN (Electronic)	9780819496218
DOIs	https://doi.org/10.1117/12.2055683
State	Published - 2014
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII - Montreal, Canada Duration: Jun 24 2014 → Jun 27 2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9153
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Country/Territory	Canada
City	Montreal
Period	6/24/14 → 6/27/14

All Science Journal Classification (ASJC) codes

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

Access to Document

10.1117/12.2055683

Cite this

Rahlin, A. S., Ade, P. A. R., Amiri, M., Benton, S. J., Bock, J. J., Bond, J. R., Bryan, S. A., Chiang, H. C., Contaldi, C. R., Crill, B. P., Doré, O., Farhang, M., Filippini, J. P., Fissel, L. M., Fraisse, A. A., Gambrel, A. E., Gandilo, N. N., Golwala, S., Gudmundsson, J. E., ... Young, E. Y. (2014). Pre-flight integration and characterization of the SPIDER balloon-borne telescope. In J. Zmuidzinas, & W. S. Holland (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII Article 915313 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9153). SPIE. https://doi.org/10.1117/12.2055683

@inproceedings{99c3ca0a46ad4a9e8740bf15cb113dcc,

title = "Pre-flight integration and characterization of the SPIDER balloon-borne telescope",

abstract = "We present the results of integration and characterization of the Spider instrument after the 2013 pre-flight campaign. Spider is a balloon-borne polarimeter designed to probe the primordial gravitational wave signal in the degree-scale B-mode polarization of the cosmic microwave background. With six independent telescopes housing over 2000 detectors in the 94 GHz and 150 GHz frequency bands, Spider will map 7.5\% of the sky with a depth of 11 to 14 μ 1/4K .arcmin at each frequency, which is a factor of ∼5 improvement over Planck. We discuss the integration of the pointing, cryogenic, electronics, and power sub-systems, as well as pre-flight characterization of the detectors and optical systems. Spider is well prepared for a December 2014 flight from Antarctica, and is expected to be limited by astrophysical foreground emission, and not instrumental sensitivity, over the survey region.",

author = "Rahlin, \{A. S.\} and Ade, \{P. A.R.\} and M. Amiri and Benton, \{S. J.\} and Bock, \{J. J.\} and Bond, \{J. R.\} and Bryan, \{S. A.\} and Chiang, \{Hsin C.\} and Contaldi, \{C. R.\} and Crill, \{B. P.\} and O. Dor{\'e} and M. Farhang and Filippini, \{J. P.\} and Fissel, \{L. M.\} and Fraisse, \{A. A.\} and Gambrel, \{A. E.\} and Gandilo, \{N. N.\} and S. Golwala and Gudmundsson, \{Jon E.\} and M. Halpern and Hasselfield, \{M. F.\} and G. Hilton and Holmes, \{W. A.\} and Hristov, \{V. V.\} and Irwin, \{K. D.\} and Jones, \{William C.\} and Kermish, \{Zigmund D.\} and Kuo, \{C. L.\} and MacTavish, \{C. J.\} and Mason, \{P. V.\} and K. Megerian and L. Moncelsi and Morford, \{T. A.\} and Nagy, \{J. M.\} and Netterfield, \{C. B.\} and R. O'Brient and C. Reintsema and Ruhl, \{J. E.\} and Runyan, \{M. C.\} and Shariff, \{J. A.\} and Soler, \{J. D.\} and A. Trangsrud and C. Tucker and Tucker, \{R. S.\} and Turner, \{A. D.\} and Weber, \{A. C.\} and Wiebe, \{D. V.\} and Young, \{E. Y.\}",

note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII ; Conference date: 24-06-2014 Through 27-06-2014",

year = "2014",

doi = "10.1117/12.2055683",

language = "English (US)",

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

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Holland, \{Wayne S.\}",

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

address = "United States",

}

Rahlin, AS, Ade, PAR, Amiri, M, Benton, SJ, Bock, JJ, Bond, JR, Bryan, SA, Chiang, HC, Contaldi, CR, Crill, BP, Doré, O, Farhang, M, Filippini, JP, Fissel, LM, Fraisse, AA, Gambrel, AE, Gandilo, NN, Golwala, S, Gudmundsson, JE, Halpern, M, Hasselfield, MF, Hilton, G, Holmes, WA, Hristov, VV, Irwin, KD, Jones, WC, Kermish, ZD, Kuo, CL, MacTavish, CJ, Mason, PV, Megerian, K, Moncelsi, L, Morford, TA, Nagy, JM, Netterfield, CB, O'Brient, R, Reintsema, C, Ruhl, JE, Runyan, MC, Shariff, JA, Soler, JD, Trangsrud, A, Tucker, C, Tucker, RS, Turner, AD, Weber, AC, Wiebe, DV & Young, EY 2014, Pre-flight integration and characterization of the SPIDER balloon-borne telescope. in J Zmuidzinas & WS Holland (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII., 915313, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9153, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, Montreal, Canada, 6/24/14. https://doi.org/10.1117/12.2055683

Pre-flight integration and characterization of the SPIDER balloon-borne telescope. / Rahlin, A. S.; Ade, P. A.R.; Amiri, M. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. ed. / Jonas Zmuidzinas; Wayne S. Holland. SPIE, 2014. 915313 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9153).

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

TY - GEN

T1 - Pre-flight integration and characterization of the SPIDER balloon-borne telescope

AU - Rahlin, A. S.

AU - Ade, P. A.R.

AU - Amiri, M.

AU - Benton, S. J.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Bryan, S. A.

AU - Chiang, Hsin C.

AU - Contaldi, C. R.

AU - Crill, B. P.

AU - Doré, O.

AU - Farhang, M.

AU - Filippini, J. P.

AU - Fissel, L. M.

AU - Fraisse, A. A.

AU - Gambrel, A. E.

AU - Gandilo, N. N.

AU - Golwala, S.

AU - Gudmundsson, Jon E.

AU - Halpern, M.

AU - Hasselfield, M. F.

AU - Hilton, G.

AU - Holmes, W. A.

AU - Hristov, V. V.

AU - Irwin, K. D.

AU - Jones, William C.

AU - Kermish, Zigmund D.

AU - Kuo, C. L.

AU - MacTavish, C. J.

AU - Mason, P. V.

AU - Megerian, K.

AU - Moncelsi, L.

AU - Morford, T. A.

AU - Nagy, J. M.

AU - Netterfield, C. B.

AU - O'Brient, R.

AU - Reintsema, C.

AU - Ruhl, J. E.

AU - Runyan, M. C.

AU - Shariff, J. A.

AU - Soler, J. D.

AU - Trangsrud, A.

AU - Tucker, C.

AU - Tucker, R. S.

AU - Turner, A. D.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Young, E. Y.

PY - 2014

Y1 - 2014

N2 - We present the results of integration and characterization of the Spider instrument after the 2013 pre-flight campaign. Spider is a balloon-borne polarimeter designed to probe the primordial gravitational wave signal in the degree-scale B-mode polarization of the cosmic microwave background. With six independent telescopes housing over 2000 detectors in the 94 GHz and 150 GHz frequency bands, Spider will map 7.5% of the sky with a depth of 11 to 14 μ 1/4K .arcmin at each frequency, which is a factor of ∼5 improvement over Planck. We discuss the integration of the pointing, cryogenic, electronics, and power sub-systems, as well as pre-flight characterization of the detectors and optical systems. Spider is well prepared for a December 2014 flight from Antarctica, and is expected to be limited by astrophysical foreground emission, and not instrumental sensitivity, over the survey region.

AB - We present the results of integration and characterization of the Spider instrument after the 2013 pre-flight campaign. Spider is a balloon-borne polarimeter designed to probe the primordial gravitational wave signal in the degree-scale B-mode polarization of the cosmic microwave background. With six independent telescopes housing over 2000 detectors in the 94 GHz and 150 GHz frequency bands, Spider will map 7.5% of the sky with a depth of 11 to 14 μ 1/4K .arcmin at each frequency, which is a factor of ∼5 improvement over Planck. We discuss the integration of the pointing, cryogenic, electronics, and power sub-systems, as well as pre-flight characterization of the detectors and optical systems. Spider is well prepared for a December 2014 flight from Antarctica, and is expected to be limited by astrophysical foreground emission, and not instrumental sensitivity, over the survey region.

UR - https://www.scopus.com/pages/publications/84921526976

UR - https://www.scopus.com/pages/publications/84921526976#tab=citedBy

U2 - 10.1117/12.2055683

DO - 10.1117/12.2055683

M3 - Conference contribution

AN - SCOPUS:84921526976

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

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

A2 - Zmuidzinas, Jonas

A2 - Holland, Wayne S.

PB - SPIE

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

Y2 - 24 June 2014 through 27 June 2014

ER -

Rahlin AS, Ade PAR, Amiri M, Benton SJ, Bock JJ, Bond JR et al. Pre-flight integration and characterization of the SPIDER balloon-borne telescope. In Zmuidzinas J, Holland WS, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. SPIE. 2014. 915313. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2055683

Pre-flight integration and characterization of the SPIDER balloon-borne telescope

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