Performance and on-sky optical characterization of the SPTpol instrument

In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camera, SPTpol, in order to measure the polarization anisotropy of the cosmic microwave background (CMB). Measurements of the polarization of the CMB at small angular scales (~several arcminutes) can detec...

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Bibliographic Details
Main Authors: George, E. M., Lueker, M., Shirokoff, E., Vieira, J. D.
Other Authors: Holland, Wayne S., Zmuidzinas, Jonas
Format: Book Part
Language:English
Published: Society of Photo-Optical Instrumentation Engineers (SPIE) 2012
Subjects:
Online Access:https://authors.library.caltech.edu/71508/
https://authors.library.caltech.edu/71508/1/84521F.pdf
https://authors.library.caltech.edu/71508/2/1210.4971v1.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723
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spelling ftcaltechauth:oai:authors.library.caltech.edu:71508 2023-05-15T18:22:50+02:00 Performance and on-sky optical characterization of the SPTpol instrument George, E. M. Lueker, M. Shirokoff, E. Vieira, J. D. Holland, Wayne S. Zmuidzinas, Jonas 2012-09-24 application/pdf https://authors.library.caltech.edu/71508/ https://authors.library.caltech.edu/71508/1/84521F.pdf https://authors.library.caltech.edu/71508/2/1210.4971v1.pdf https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723 en eng Society of Photo-Optical Instrumentation Engineers (SPIE) https://authors.library.caltech.edu/71508/1/84521F.pdf https://authors.library.caltech.edu/71508/2/1210.4971v1.pdf George, E. M. and Lueker, M. and Shirokoff, E. and Vieira, J. D. (2012) Performance and on-sky optical characterization of the SPTpol instrument. In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI. Proceedings of SPIE. No.8452. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 84521F. ISBN 978-0-8194-9153-4. https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723 <https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723> other Book Section PeerReviewed 2012 ftcaltechauth 2021-11-18T18:39:32Z In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camera, SPTpol, in order to measure the polarization anisotropy of the cosmic microwave background (CMB). Measurements of the polarization of the CMB at small angular scales (~several arcminutes) can detect the gravitational lensing of the CMB by large scale structure and constrain the sum of the neutrino masses. At large angular scales (~few degrees) CMB measurements can constrain the energy scale of Inflation. SPTpol is a two-color mm-wave camera that consists of 180 polarimeters at 90 GHz and 588 polarimeters at 150 GHz, with each polarimeter consisting of a dual transition edge sensor (TES) bolometers. The full complement of 150 GHz detectors consists of 7 arrays of 84 ortho-mode transducers (OMTs) that are stripline coupled to two TES detectors per OMT, developed by the TRUCE collaboration and fabricated at NIST. Each 90 GHz pixel consists of two antenna-coupled absorbers coupled to two TES detectors, developed with Argonne National Labs. The 1536 total detectors are read out with digital frequency-domain multiplexing (DfMUX). The SPTpol deployment represents the first on-sky tests of both of these detector technologies, and is one of the first deployed instruments using DfMUX readout technology. We present the details of the design, commissioning, deployment, on-sky optical characterization and detector performance of the complete SPTpol focal plane. Book Part South pole Caltech Authors (California Institute of Technology) South Pole
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language English
description In January 2012, the 10m South Pole Telescope (SPT) was equipped with a polarization-sensitive camera, SPTpol, in order to measure the polarization anisotropy of the cosmic microwave background (CMB). Measurements of the polarization of the CMB at small angular scales (~several arcminutes) can detect the gravitational lensing of the CMB by large scale structure and constrain the sum of the neutrino masses. At large angular scales (~few degrees) CMB measurements can constrain the energy scale of Inflation. SPTpol is a two-color mm-wave camera that consists of 180 polarimeters at 90 GHz and 588 polarimeters at 150 GHz, with each polarimeter consisting of a dual transition edge sensor (TES) bolometers. The full complement of 150 GHz detectors consists of 7 arrays of 84 ortho-mode transducers (OMTs) that are stripline coupled to two TES detectors per OMT, developed by the TRUCE collaboration and fabricated at NIST. Each 90 GHz pixel consists of two antenna-coupled absorbers coupled to two TES detectors, developed with Argonne National Labs. The 1536 total detectors are read out with digital frequency-domain multiplexing (DfMUX). The SPTpol deployment represents the first on-sky tests of both of these detector technologies, and is one of the first deployed instruments using DfMUX readout technology. We present the details of the design, commissioning, deployment, on-sky optical characterization and detector performance of the complete SPTpol focal plane.
author2 Holland, Wayne S.
Zmuidzinas, Jonas
format Book Part
author George, E. M.
Lueker, M.
Shirokoff, E.
Vieira, J. D.
spellingShingle George, E. M.
Lueker, M.
Shirokoff, E.
Vieira, J. D.
Performance and on-sky optical characterization of the SPTpol instrument
author_facet George, E. M.
Lueker, M.
Shirokoff, E.
Vieira, J. D.
author_sort George, E. M.
title Performance and on-sky optical characterization of the SPTpol instrument
title_short Performance and on-sky optical characterization of the SPTpol instrument
title_full Performance and on-sky optical characterization of the SPTpol instrument
title_fullStr Performance and on-sky optical characterization of the SPTpol instrument
title_full_unstemmed Performance and on-sky optical characterization of the SPTpol instrument
title_sort performance and on-sky optical characterization of the sptpol instrument
publisher Society of Photo-Optical Instrumentation Engineers (SPIE)
publishDate 2012
url https://authors.library.caltech.edu/71508/
https://authors.library.caltech.edu/71508/1/84521F.pdf
https://authors.library.caltech.edu/71508/2/1210.4971v1.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://authors.library.caltech.edu/71508/1/84521F.pdf
https://authors.library.caltech.edu/71508/2/1210.4971v1.pdf
George, E. M. and Lueker, M. and Shirokoff, E. and Vieira, J. D. (2012) Performance and on-sky optical characterization of the SPTpol instrument. In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI. Proceedings of SPIE. No.8452. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 84521F. ISBN 978-0-8194-9153-4. https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723 <https://resolver.caltech.edu/CaltechAUTHORS:20161026-141054723>
op_rights other
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