Modeling and characterization of the SPIDER half-wave plate

Sean A. Bryan; Peter A.R. Ade; Mandana Amiri; Steve Benton; Richard Bihary; James J. Bock; J. Richard Bond; Joseph A. Bonetti; H. Cynthia Chiang; Carlo R. Contaldi; Brendan P. Crill; Daniel O'Dea; Olivier Dore; Marzieh Farhang; Jeffrey P. Filippini; Laura Fissel; Natalie Gandilo; Sunil Golwala; Jon E. Gudmundsson; Matthew Hasselfield; Mark Halpern; Kyle R. Helson; Gene Hilton; Warren Holmes; Viktor V. Hristov; Kent D. Irwin; William C. Jones; Chao Lin Kuo; Carrie J. MacTavish; Peter Mason; Tracy Morford; Thomas E. Montroy; C. Barth Netterfield; Alexandra S. Rahlin; Carl D. Reintsema; Daniel Riley; John E. Ruhl; Marcus C. Runyan; Matthew A. Schenker; Jamil Shariff; Juan Diego Soler; Amy Transrud; Rebecca Tucker; Carole Tucker; Anthony Turner

doi:10.1117/12.857837

Modeling and characterization of the SPIDER half-wave plate

Sean A. Bryan, Peter A.R. Ade, Mandana Amiri, Steve Benton, Richard Bihary, James J. Bock, J. Richard Bond, Joseph A. Bonetti, H. Cynthia Chiang, Carlo R. Contaldi, Brendan P. Crill, Daniel O'Dea, Olivier Dore, Marzieh Farhang, Jeffrey P. Filippini, Laura Fissel, Natalie Gandilo, Sunil Golwala, Jon E. Gudmundsson, Matthew HasselfieldMark Halpern, Kyle R. Helson, Gene Hilton, Warren Holmes, Viktor V. Hristov, Kent D. Irwin, William C. Jones, Chao Lin Kuo, Carrie J. MacTavish, Peter Mason, Tracy Morford, Thomas E. Montroy, C. Barth Netterfield, Alexandra S. Rahlin, Carl D. Reintsema, Daniel Riley, John E. Ruhl, Marcus C. Runyan, Matthew A. Schenker, Jamil Shariff, Juan Diego Soler, Amy Transrud, Rebecca Tucker, Carole Tucker, Anthony Turner

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

25 Scopus citations

Abstract

Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization map of the CMB with approximately one-half degree resolution at 145 GHz. Polarization modulation is achieved via a cryogenic sapphire half-wave plate (HWP) skyward of the primary optic. We have measured millimeter-wave transmission spectra of the sapphire at room and cryogenic temperatures. The spectra are consistent with our physical optics model, and the data gives excellent measurements of the indices of A-cut sapphire. We have also taken preliminary spectra of the integrated HWP, optical system, and detectors in the prototype Spider receiver. We calculate the variation in response of the HWP between observing the CMB and foreground spectra, and estimate that it should not limit the Spider constraints on inflation.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
DOIs	https://doi.org/10.1117/12.857837
State	Published - 2010
Externally published	Yes
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V - San Diego, CA, United States Duration: Jun 29 2010 → Jul 2 2010

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7741
ISSN (Print)	0277-786X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V
Country/Territory	United States
City	San Diego, CA
Period	6/29/10 → 7/2/10

Keywords

Astronomical polarimetry
Cosmic Microwave Background
Cosmology
Millimeter-wave optics

ASJC Scopus subject areas

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

Access to Document

10.1117/12.857837

Cite this

Bryan, S. A., Ade, P. A. R., Amiri, M., Benton, S., Bihary, R., Bock, J. J., Bond, J. R., Bonetti, J. A., Chiang, H. C., Contaldi, C. R., Crill, B. P., O'Dea, D., Dore, O., Farhang, M., Filippini, J. P., Fissel, L., Gandilo, N., Golwala, S., Gudmundsson, J. E., ... Turner, A. (2010). Modeling and characterization of the SPIDER half-wave plate. In Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V Article 77412B (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7741). https://doi.org/10.1117/12.857837

Modeling and characterization of the SPIDER half-wave plate. / Bryan, Sean A.; Ade, Peter A.R.; Amiri, Mandana et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V. 2010. 77412B (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7741).

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

Bryan, SA, Ade, PAR, Amiri, M, Benton, S, Bihary, R, Bock, JJ, Bond, JR, Bonetti, JA, Chiang, HC, Contaldi, CR, Crill, BP, O'Dea, D, Dore, O, Farhang, M, Filippini, JP, Fissel, L, Gandilo, N, Golwala, S, Gudmundsson, JE, Hasselfield, M, Halpern, M, Helson, KR, Hilton, G, Holmes, W, Hristov, VV, Irwin, KD, Jones, WC, Kuo, CL, MacTavish, CJ, Mason, P, Morford, T, Montroy, TE, Netterfield, CB, Rahlin, AS, Reintsema, CD, Riley, D, Ruhl, JE, Runyan, MC, Schenker, MA, Shariff, J, Soler, JD, Transrud, A, Tucker, R, Tucker, C & Turner, A 2010, Modeling and characterization of the SPIDER half-wave plate. in Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V., 77412B, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7741, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V, San Diego, CA, United States, 6/29/10. https://doi.org/10.1117/12.857837

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title = "Modeling and characterization of the SPIDER half-wave plate",

abstract = "Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization map of the CMB with approximately one-half degree resolution at 145 GHz. Polarization modulation is achieved via a cryogenic sapphire half-wave plate (HWP) skyward of the primary optic. We have measured millimeter-wave transmission spectra of the sapphire at room and cryogenic temperatures. The spectra are consistent with our physical optics model, and the data gives excellent measurements of the indices of A-cut sapphire. We have also taken preliminary spectra of the integrated HWP, optical system, and detectors in the prototype Spider receiver. We calculate the variation in response of the HWP between observing the CMB and foreground spectra, and estimate that it should not limit the Spider constraints on inflation.",

keywords = "Astronomical polarimetry, Cosmic Microwave Background, Cosmology, Millimeter-wave optics",

author = "Bryan, {Sean A.} and Ade, {Peter A.R.} and Mandana Amiri and Steve Benton and Richard Bihary and Bock, {James J.} and Bond, {J. Richard} and Bonetti, {Joseph A.} and Chiang, {H. Cynthia} and Contaldi, {Carlo R.} and Crill, {Brendan P.} and Daniel O'Dea and Olivier Dore and Marzieh Farhang and Filippini, {Jeffrey P.} and Laura Fissel and Natalie Gandilo and Sunil Golwala and Gudmundsson, {Jon E.} and Matthew Hasselfield and Mark Halpern and Helson, {Kyle R.} and Gene Hilton and Warren Holmes and Hristov, {Viktor V.} and Irwin, {Kent D.} and Jones, {William C.} and Kuo, {Chao Lin} and MacTavish, {Carrie J.} and Peter Mason and Tracy Morford and Montroy, {Thomas E.} and Netterfield, {C. Barth} and Rahlin, {Alexandra S.} and Reintsema, {Carl D.} and Daniel Riley and Ruhl, {John E.} and Runyan, {Marcus C.} and Schenker, {Matthew A.} and Jamil Shariff and Soler, {Juan Diego} and Amy Transrud and Rebecca Tucker and Carole Tucker and Anthony Turner",

year = "2010",

doi = "10.1117/12.857837",

language = "English (US)",

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TY - GEN

T1 - Modeling and characterization of the SPIDER half-wave plate

AU - Bryan, Sean A.

AU - Ade, Peter A.R.

AU - Amiri, Mandana

AU - Benton, Steve

AU - Bihary, Richard

AU - Bock, James J.

AU - Bond, J. Richard

AU - Bonetti, Joseph A.

AU - Chiang, H. Cynthia

AU - Contaldi, Carlo R.

AU - Crill, Brendan P.

AU - O'Dea, Daniel

AU - Dore, Olivier

AU - Farhang, Marzieh

AU - Filippini, Jeffrey P.

AU - Fissel, Laura

AU - Gandilo, Natalie

AU - Golwala, Sunil

AU - Gudmundsson, Jon E.

AU - Hasselfield, Matthew

AU - Halpern, Mark

AU - Helson, Kyle R.

AU - Hilton, Gene

AU - Holmes, Warren

AU - Hristov, Viktor V.

AU - Irwin, Kent D.

AU - Jones, William C.

AU - Kuo, Chao Lin

AU - MacTavish, Carrie J.

AU - Mason, Peter

AU - Morford, Tracy

AU - Montroy, Thomas E.

AU - Netterfield, C. Barth

AU - Rahlin, Alexandra S.

AU - Reintsema, Carl D.

AU - Riley, Daniel

AU - Ruhl, John E.

AU - Runyan, Marcus C.

AU - Schenker, Matthew A.

AU - Shariff, Jamil

AU - Soler, Juan Diego

AU - Transrud, Amy

AU - Tucker, Rebecca

AU - Tucker, Carole

AU - Turner, Anthony

PY - 2010

Y1 - 2010

N2 - Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization map of the CMB with approximately one-half degree resolution at 145 GHz. Polarization modulation is achieved via a cryogenic sapphire half-wave plate (HWP) skyward of the primary optic. We have measured millimeter-wave transmission spectra of the sapphire at room and cryogenic temperatures. The spectra are consistent with our physical optics model, and the data gives excellent measurements of the indices of A-cut sapphire. We have also taken preliminary spectra of the integrated HWP, optical system, and detectors in the prototype Spider receiver. We calculate the variation in response of the HWP between observing the CMB and foreground spectra, and estimate that it should not limit the Spider constraints on inflation.

AB - Spider is a balloon-borne array of six telescopes that will observe the Cosmic Microwave Background. The 2624 antenna-coupled bolometers in the instrument will make a polarization map of the CMB with approximately one-half degree resolution at 145 GHz. Polarization modulation is achieved via a cryogenic sapphire half-wave plate (HWP) skyward of the primary optic. We have measured millimeter-wave transmission spectra of the sapphire at room and cryogenic temperatures. The spectra are consistent with our physical optics model, and the data gives excellent measurements of the indices of A-cut sapphire. We have also taken preliminary spectra of the integrated HWP, optical system, and detectors in the prototype Spider receiver. We calculate the variation in response of the HWP between observing the CMB and foreground spectra, and estimate that it should not limit the Spider constraints on inflation.

KW - Astronomical polarimetry

KW - Cosmic Microwave Background

KW - Cosmology

KW - Millimeter-wave optics

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U2 - 10.1117/12.857837

DO - 10.1117/12.857837

M3 - Conference contribution

AN - SCOPUS:77956205758

SN - 9780819482310

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

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

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

Y2 - 29 June 2010 through 2 July 2010

ER -

Modeling and characterization of the SPIDER half-wave plate

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Keywords

ASJC Scopus subject areas

Access to Document

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