QUEST on DASI: A South Pole CMB polarization experiment

Sarah Church; Peter Ade; James Bock; Melanie Bowden; John Carlstrom; Ken Ganga; Walter Gear; James Hinderks; Wayne Hu; Brian Keating; John Kovac; Andrew Lange; Eric Leitch; Olivier Mallie; Simon Melhuish; Anthony Murphy; Ben Rusholme; Creidhe O'Sullivan; Lucio Piccirillo; Clem Pryke; Andy Taylor; Keith Thompson

doi:10.1016/j.newar.2003.09.033

QUEST on DASI: A South Pole CMB polarization experiment

Sarah Church
, Peter Ade
, James Bock
, Melanie Bowden
, John Carlstrom
, Ken Ganga
, Walter Gear
, James Hinderks
, Wayne Hu
, Brian Keating
, John Kovac
, Andrew Lange
, Eric Leitch
, Olivier Mallie
, Simon Melhuish
, Anthony Murphy
, Ben Rusholme
, Creidhe O'Sullivan
, Lucio Piccirillo
, Clem Pryke

Andy Taylor, Keith Thompson

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Short survey › peer-review

30 Scopus citations

Abstract

QUEST on DASI is a ground-based, high-sensitivity, high-resolution (ℓ_max∼2500) experiment designed to map CMB polarization at 100 and 150 GHz and to measure the power spectra from E-modes, B-modes from lensing of the CMB, and B-modes from primordial gravitational waves. The experiment comprises a 2.6 m Cassegrain optical system, equipped with an array of 62 polarization-sensitive bolometers (PSBs), located at the South Pole. The instrument is designed to minimize systematic effects; features include differencing of pairs of orthogonal PSBs within a single feed, a rotatable achromatic waveplate, and axisymmetric rotatable optics. In addition the South Pole location allows both repeatable and highly controlled observations. QUEST on DASI will commence operation in early 2005.

Original language	English (US)
Pages (from-to)	1083-1089
Number of pages	7
Journal	New Astronomy Reviews
Volume	47
Issue number	11-12
DOIs	https://doi.org/10.1016/j.newar.2003.09.033
State	Published - Dec 2003

Bibliographical note

Funding Information:
This material is based upon work supported by the National Science Foundation under Grants 9987360 and 0096778, by the Particle Physics and Astronomy Research Council in the UK, and by the Irish Research Council for Science, Engineering and Technology.

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10.1016/j.newar.2003.09.033

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Church, S., Ade, P., Bock, J., Bowden, M., Carlstrom, J., Ganga, K., Gear, W., Hinderks, J., Hu, W., Keating, B., Kovac, J., Lange, A., Leitch, E., Mallie, O., Melhuish, S., Murphy, A., Rusholme, B., O'Sullivan, C., Piccirillo, L., ... Thompson, K. (2003). QUEST on DASI: A South Pole CMB polarization experiment. New Astronomy Reviews, 47(11-12), 1083-1089. https://doi.org/10.1016/j.newar.2003.09.033

Church, S, Ade, P, Bock, J, Bowden, M, Carlstrom, J, Ganga, K, Gear, W, Hinderks, J, Hu, W, Keating, B, Kovac, J, Lange, A, Leitch, E, Mallie, O, Melhuish, S, Murphy, A, Rusholme, B, O'Sullivan, C, Piccirillo, L, Pryke, C, Taylor, A & Thompson, K 2003, 'QUEST on DASI: A South Pole CMB polarization experiment', New Astronomy Reviews, vol. 47, no. 11-12, pp. 1083-1089. https://doi.org/10.1016/j.newar.2003.09.033

@article{0edb4a48c9e2458d88f73a67c48bbe1c,

title = "QUEST on DASI: A South Pole CMB polarization experiment",

abstract = "QUEST on DASI is a ground-based, high-sensitivity, high-resolution (ℓmax∼2500) experiment designed to map CMB polarization at 100 and 150 GHz and to measure the power spectra from E-modes, B-modes from lensing of the CMB, and B-modes from primordial gravitational waves. The experiment comprises a 2.6 m Cassegrain optical system, equipped with an array of 62 polarization-sensitive bolometers (PSBs), located at the South Pole. The instrument is designed to minimize systematic effects; features include differencing of pairs of orthogonal PSBs within a single feed, a rotatable achromatic waveplate, and axisymmetric rotatable optics. In addition the South Pole location allows both repeatable and highly controlled observations. QUEST on DASI will commence operation in early 2005.",

author = "Sarah Church and Peter Ade and James Bock and Melanie Bowden and John Carlstrom and Ken Ganga and Walter Gear and James Hinderks and Wayne Hu and Brian Keating and John Kovac and Andrew Lange and Eric Leitch and Olivier Mallie and Simon Melhuish and Anthony Murphy and Ben Rusholme and Creidhe O'Sullivan and Lucio Piccirillo and Clem Pryke and Andy Taylor and Keith Thompson",

note = "Funding Information: This material is based upon work supported by the National Science Foundation under Grants 9987360 and 0096778, by the Particle Physics and Astronomy Research Council in the UK, and by the Irish Research Council for Science, Engineering and Technology. ",

year = "2003",

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doi = "10.1016/j.newar.2003.09.033",

language = "English (US)",

volume = "47",

pages = "1083--1089",

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T1 - QUEST on DASI

T2 - A South Pole CMB polarization experiment

AU - Church, Sarah

AU - Ade, Peter

AU - Bock, James

AU - Bowden, Melanie

AU - Carlstrom, John

AU - Ganga, Ken

AU - Gear, Walter

AU - Hinderks, James

AU - Hu, Wayne

AU - Keating, Brian

AU - Kovac, John

AU - Lange, Andrew

AU - Leitch, Eric

AU - Mallie, Olivier

AU - Melhuish, Simon

AU - Murphy, Anthony

AU - Rusholme, Ben

AU - O'Sullivan, Creidhe

AU - Piccirillo, Lucio

AU - Pryke, Clem

AU - Taylor, Andy

AU - Thompson, Keith

N1 - Funding Information: This material is based upon work supported by the National Science Foundation under Grants 9987360 and 0096778, by the Particle Physics and Astronomy Research Council in the UK, and by the Irish Research Council for Science, Engineering and Technology.

PY - 2003/12

Y1 - 2003/12

N2 - QUEST on DASI is a ground-based, high-sensitivity, high-resolution (ℓmax∼2500) experiment designed to map CMB polarization at 100 and 150 GHz and to measure the power spectra from E-modes, B-modes from lensing of the CMB, and B-modes from primordial gravitational waves. The experiment comprises a 2.6 m Cassegrain optical system, equipped with an array of 62 polarization-sensitive bolometers (PSBs), located at the South Pole. The instrument is designed to minimize systematic effects; features include differencing of pairs of orthogonal PSBs within a single feed, a rotatable achromatic waveplate, and axisymmetric rotatable optics. In addition the South Pole location allows both repeatable and highly controlled observations. QUEST on DASI will commence operation in early 2005.

AB - QUEST on DASI is a ground-based, high-sensitivity, high-resolution (ℓmax∼2500) experiment designed to map CMB polarization at 100 and 150 GHz and to measure the power spectra from E-modes, B-modes from lensing of the CMB, and B-modes from primordial gravitational waves. The experiment comprises a 2.6 m Cassegrain optical system, equipped with an array of 62 polarization-sensitive bolometers (PSBs), located at the South Pole. The instrument is designed to minimize systematic effects; features include differencing of pairs of orthogonal PSBs within a single feed, a rotatable achromatic waveplate, and axisymmetric rotatable optics. In addition the South Pole location allows both repeatable and highly controlled observations. QUEST on DASI will commence operation in early 2005.

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DO - 10.1016/j.newar.2003.09.033

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AN - SCOPUS:0344392741

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SP - 1083

EP - 1089

JO - New Astronomy Reviews

JF - New Astronomy Reviews

IS - 11-12

ER -

QUEST on DASI: A South Pole CMB polarization experiment

Abstract

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