SPIDER: A balloon-borne large-scale Cmb polarimeter

B. P. Crill; P. A.R. Ade; E. S. Battistelli; S. Benton; R. Bihary; J. J. Bock; J. R. Bond; J. Brevik; S. Bryan; C. R. Contaldi; O. Doré; M. Farhang; L. Fissel; S. R. Golwala; M. Halpern; G. Hilton; W. Holmes; V. V. Hristov; K. Irwin; W. C. Jones; C. L. Kuo; A. E. Lange; C. Lawrie; C. J. MacTavish; T. G. Martin; P. Mason; T. E. Montroy; C. B. Netterfield; E. Pascale; D. Riley; J. E. Ruhl; M. C. Runyan; A. Trangsrud; C. Tucker; A. Turner; M. Viero; D. Wiebe

doi:10.1117/12.787446

SPIDER: A balloon-borne large-scale Cmb polarimeter

B. P. Crill, P. A.R. Ade, E. S. Battistelli, S. Benton, R. Bihary, J. J. Bock, J. R. Bond, J. Brevik, S. Bryan, C. R. Contaldi, O. Doré, M. Farhang, L. Fissel, S. R. Golwala, M. Halpern, G. Hilton, W. Holmes, V. V. Hristov, K. Irwin, W. C. JonesC. L. Kuo, A. E. Lange, C. Lawrie, C. J. MacTavish, T. G. Martin, P. Mason, T. E. Montroy, C. B. Netterfield, E. Pascale, D. Riley, J. E. Ruhl, M. C. Runyan, A. Trangsrud, C. Tucker, A. Turner, M. Viero, D. Wiebe

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

51 Scopus citations

Abstract

SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ∼ 1° resolution. Six monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities of 4.2 and 3.1 μK_CMB √s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs, Australia in 2010, SPIDER will map 50% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor.

Original language	English (US)
Title of host publication	Space Telescopes and Instrumentation 2008
Subtitle of host publication	Optical, Infrared, and Millimeter
DOIs	https://doi.org/10.1117/12.787446
State	Published - 2008
Externally published	Yes
Event	Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter - Marseille, France Duration: Jun 23 2008 → Jun 28 2008

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7010
ISSN (Print)	0277-786X

Other

Other	Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Country/Territory	France
City	Marseille
Period	6/23/08 → 6/28/08

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

10.1117/12.787446

Cite this

Crill, B. P., Ade, P. A. R., Battistelli, E. S., Benton, S., Bihary, R., Bock, J. J., Bond, J. R., Brevik, J., Bryan, S., Contaldi, C. R., Doré, O., Farhang, M., Fissel, L., Golwala, S. R., Halpern, M., Hilton, G., Holmes, W., Hristov, V. V., Irwin, K., ... Wiebe, D. (2008). SPIDER: A balloon-borne large-scale Cmb polarimeter. In Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter Article 70102P (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7010). https://doi.org/10.1117/12.787446

@inproceedings{d1a44a863008462fbf85023693dd7c4d,

title = "SPIDER: A balloon-borne large-scale Cmb polarimeter",

abstract = "SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ∼ 1° resolution. Six monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities of 4.2 and 3.1 μKCMB √s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs, Australia in 2010, SPIDER will map 50\% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor.",

author = "Crill, \{B. P.\} and Ade, \{P. A.R.\} and Battistelli, \{E. S.\} and S. Benton and R. Bihary and Bock, \{J. J.\} and Bond, \{J. R.\} and J. Brevik and S. Bryan and Contaldi, \{C. R.\} and O. Dor{\'e} and M. Farhang and L. Fissel and Golwala, \{S. R.\} and M. Halpern and G. Hilton and W. Holmes and Hristov, \{V. V.\} and K. Irwin and Jones, \{W. C.\} and Kuo, \{C. L.\} and Lange, \{A. E.\} and C. Lawrie and MacTavish, \{C. J.\} and Martin, \{T. G.\} and P. Mason and Montroy, \{T. E.\} and Netterfield, \{C. B.\} and E. Pascale and D. Riley and Ruhl, \{J. E.\} and Runyan, \{M. C.\} and A. Trangsrud and C. Tucker and A. Turner and M. Viero and D. Wiebe",

year = "2008",

doi = "10.1117/12.787446",

language = "English (US)",

isbn = "9780819472205",

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

booktitle = "Space Telescopes and Instrumentation 2008",

note = "Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter ; Conference date: 23-06-2008 Through 28-06-2008",

}

Crill, BP, Ade, PAR, Battistelli, ES, Benton, S, Bihary, R, Bock, JJ, Bond, JR, Brevik, J, Bryan, S, Contaldi, CR, Doré, O, Farhang, M, Fissel, L, Golwala, SR, Halpern, M, Hilton, G, Holmes, W, Hristov, VV, Irwin, K, Jones, WC, Kuo, CL, Lange, AE, Lawrie, C, MacTavish, CJ, Martin, TG, Mason, P, Montroy, TE, Netterfield, CB, Pascale, E, Riley, D, Ruhl, JE, Runyan, MC, Trangsrud, A, Tucker, C, Turner, A, Viero, M & Wiebe, D 2008, SPIDER: A balloon-borne large-scale Cmb polarimeter. in Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter., 70102P, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, Marseille, France, 6/23/08. https://doi.org/10.1117/12.787446

SPIDER: A balloon-borne large-scale Cmb polarimeter. / Crill, B. P.; Ade, P. A.R.; Battistelli, E. S. et al.
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter. 2008. 70102P (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7010).

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

TY - GEN

T1 - SPIDER

T2 - Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter

AU - Crill, B. P.

AU - Ade, P. A.R.

AU - Battistelli, E. S.

AU - Benton, S.

AU - Bihary, R.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Brevik, J.

AU - Bryan, S.

AU - Contaldi, C. R.

AU - Doré, O.

AU - Farhang, M.

AU - Fissel, L.

AU - Golwala, S. R.

AU - Halpern, M.

AU - Hilton, G.

AU - Holmes, W.

AU - Hristov, V. V.

AU - Irwin, K.

AU - Jones, W. C.

AU - Kuo, C. L.

AU - Lange, A. E.

AU - Lawrie, C.

AU - MacTavish, C. J.

AU - Martin, T. G.

AU - Mason, P.

AU - Montroy, T. E.

AU - Netterfield, C. B.

AU - Pascale, E.

AU - Riley, D.

AU - Ruhl, J. E.

AU - Runyan, M. C.

AU - Trangsrud, A.

AU - Tucker, C.

AU - Turner, A.

AU - Viero, M.

AU - Wiebe, D.

PY - 2008

Y1 - 2008

N2 - SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ∼ 1° resolution. Six monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities of 4.2 and 3.1 μKCMB √s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs, Australia in 2010, SPIDER will map 50% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor.

AB - SPIDER is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ∼ 1° resolution. Six monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities of 4.2 and 3.1 μKCMB √s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs, Australia in 2010, SPIDER will map 50% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor.

UR - https://www.scopus.com/pages/publications/70349516291

UR - https://www.scopus.com/inward/citedby.url?scp=70349516291&partnerID=8YFLogxK

U2 - 10.1117/12.787446

DO - 10.1117/12.787446

M3 - Conference contribution

AN - SCOPUS:70349516291

SN - 9780819472205

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

BT - Space Telescopes and Instrumentation 2008

Y2 - 23 June 2008 through 28 June 2008

ER -

SPIDER: A balloon-borne large-scale Cmb polarimeter

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