Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry

J. Hubmayr; J. Austermann; J. Beall; D. Becker; H. M. Cho; R. Datta; S. M. Duff; E. Grace; N. Halverson; S. W. Henderson; G. C. Hilton; S. P. Ho; K. D. Irwin; B. J. Koopman; D. Li; J. Mcmahon; C. Munson; M. D. Niemack; C. Pappas; B. L. Schmitt; S. M. Simon; S. T. Staggs; J. Van Lanen; E. Wollack

Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry

J. Hubmayr
, J. Austermann
, J. Beall
, D. Becker
, H. M. Cho
, R. Datta
, S. M. Duff
, E. Grace
, N. Halverson
, S. W. Henderson
, G. C. Hilton
, S. P. Ho
, K. D. Irwin
, B. J. Koopman
, D. Li
, J. Mcmahon
, C. Munson
, M. D. Niemack
, C. Pappas
, B. L. Schmitt

S. M. Simon, S. T. Staggs, J. Van Lanen, E. Wollack

Research output: Contribution to conference › Paper › peer-review

1 Scopus citations

Abstract

NIST produces large-format, dual-polarizationsensitive detector arrays for a broad range of frequencies (30-1400 GHz). Such arrays enable a host of astrophysical measurements. Detectors optimized for cosmic microwave background observations are monolithic, polarization-sensitive arrays based on feedhorn and planar Nb antenna-coupled transitionedge superconducting (TES) bolometers. Recent designs achieve multiband, polarimetric sensing within each spatial pixel. In this proceeding, we describe our multichroic, feedhorn-coupled design; demonstrate performance at 70-380 GHz; and comment on current developments for implementation of these detector arrays in the advanced Atacama Cosmology Telescope receiver.

Original language	English (US)
State	Published - 2015
Event	26th International Symposium on Space Terahertz Technology, ISSTT 2015 - Cambridge, United States Duration: Mar 16 2015 → Mar 18 2015

Other

Other	26th International Symposium on Space Terahertz Technology, ISSTT 2015
Country/Territory	United States
City	Cambridge
Period	3/16/15 → 3/18/15

All Science Journal Classification (ASJC) codes

Radiation
Electrical and Electronic Engineering
Computer Networks and Communications
Atomic and Molecular Physics, and Optics
Space and Planetary Science

Cite this

Hubmayr, J., Austermann, J., Beall, J., Becker, D., Cho, H. M., Datta, R., Duff, S. M., Grace, E., Halverson, N., Henderson, S. W., Hilton, G. C., Ho, S. P., Irwin, K. D., Koopman, B. J., Li, D., Mcmahon, J., Munson, C., Niemack, M. D., Pappas, C., ... Wollack, E. (2015). Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry. Paper presented at 26th International Symposium on Space Terahertz Technology, ISSTT 2015, Cambridge, United States.

@conference{87f560bc2559415cb5e243976c84aa8b,

title = "Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry",

abstract = "NIST produces large-format, dual-polarizationsensitive detector arrays for a broad range of frequencies (30-1400 GHz). Such arrays enable a host of astrophysical measurements. Detectors optimized for cosmic microwave background observations are monolithic, polarization-sensitive arrays based on feedhorn and planar Nb antenna-coupled transitionedge superconducting (TES) bolometers. Recent designs achieve multiband, polarimetric sensing within each spatial pixel. In this proceeding, we describe our multichroic, feedhorn-coupled design; demonstrate performance at 70-380 GHz; and comment on current developments for implementation of these detector arrays in the advanced Atacama Cosmology Telescope receiver.",

author = "J. Hubmayr and J. Austermann and J. Beall and D. Becker and Cho, \{H. M.\} and R. Datta and Duff, \{S. M.\} and E. Grace and N. Halverson and Henderson, \{S. W.\} and Hilton, \{G. C.\} and Ho, \{S. P.\} and Irwin, \{K. D.\} and Koopman, \{B. J.\} and D. Li and J. Mcmahon and C. Munson and Niemack, \{M. D.\} and C. Pappas and Schmitt, \{B. L.\} and Simon, \{S. M.\} and Staggs, \{S. T.\} and \{Van Lanen\}, J. and E. Wollack",

year = "2015",

language = "English (US)",

note = "26th International Symposium on Space Terahertz Technology, ISSTT 2015 ; Conference date: 16-03-2015 Through 18-03-2015",

}

Hubmayr, J, Austermann, J, Beall, J, Becker, D, Cho, HM, Datta, R, Duff, SM, Grace, E, Halverson, N, Henderson, SW, Hilton, GC, Ho, SP, Irwin, KD, Koopman, BJ, Li, D, Mcmahon, J, Munson, C, Niemack, MD, Pappas, C, Schmitt, BL, Simon, SM, Staggs, ST, Van Lanen, J & Wollack, E 2015, 'Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry', Paper presented at 26th International Symposium on Space Terahertz Technology, ISSTT 2015, Cambridge, United States, 3/16/15 - 3/18/15.

TY - CONF

T1 - Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry

AU - Hubmayr, J.

AU - Austermann, J.

AU - Beall, J.

AU - Becker, D.

AU - Cho, H. M.

AU - Datta, R.

AU - Duff, S. M.

AU - Grace, E.

AU - Halverson, N.

AU - Henderson, S. W.

AU - Hilton, G. C.

AU - Ho, S. P.

AU - Irwin, K. D.

AU - Koopman, B. J.

AU - Li, D.

AU - Mcmahon, J.

AU - Munson, C.

AU - Niemack, M. D.

AU - Pappas, C.

AU - Schmitt, B. L.

AU - Simon, S. M.

AU - Staggs, S. T.

AU - Van Lanen, J.

AU - Wollack, E.

PY - 2015

Y1 - 2015

N2 - NIST produces large-format, dual-polarizationsensitive detector arrays for a broad range of frequencies (30-1400 GHz). Such arrays enable a host of astrophysical measurements. Detectors optimized for cosmic microwave background observations are monolithic, polarization-sensitive arrays based on feedhorn and planar Nb antenna-coupled transitionedge superconducting (TES) bolometers. Recent designs achieve multiband, polarimetric sensing within each spatial pixel. In this proceeding, we describe our multichroic, feedhorn-coupled design; demonstrate performance at 70-380 GHz; and comment on current developments for implementation of these detector arrays in the advanced Atacama Cosmology Telescope receiver.

AB - NIST produces large-format, dual-polarizationsensitive detector arrays for a broad range of frequencies (30-1400 GHz). Such arrays enable a host of astrophysical measurements. Detectors optimized for cosmic microwave background observations are monolithic, polarization-sensitive arrays based on feedhorn and planar Nb antenna-coupled transitionedge superconducting (TES) bolometers. Recent designs achieve multiband, polarimetric sensing within each spatial pixel. In this proceeding, we describe our multichroic, feedhorn-coupled design; demonstrate performance at 70-380 GHz; and comment on current developments for implementation of these detector arrays in the advanced Atacama Cosmology Telescope receiver.

UR - https://www.scopus.com/pages/publications/84947220782

UR - https://www.scopus.com/pages/publications/84947220782#tab=citedBy

M3 - Paper

AN - SCOPUS:84947220782

T2 - 26th International Symposium on Space Terahertz Technology, ISSTT 2015

Y2 - 16 March 2015 through 18 March 2015

ER -

Feedhorn-Coupled transition-edge superconducting bolometer arrays for cosmic microwave background Polarimetry

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All Science Journal Classification (ASJC) codes

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