BICEP3 performance overview and planned Keck Array upgrade

J. A. Grayson; P. A.R. Ade; Z. Ahmed; K. D. Alexander; M. Amiri; D. Barkats; S. J. Benton; C. A. Bischoff; J. J. Bock; H. Boenish; R. Bowens-Rubin; I. Buder; E. Bullock; V. Buza; J. Connors; J. P. Filippini; S. Fliescher; M. Halpern; S. Harrison; G. C. Hilton; V. V. Hristov; H. Hui; K. D. Irwin; J. Kang; K. S. Karkare; E. Karpel; S. Kefeli; S. A. Kernasovskiy; J. M. Kovac; C. L. Kuo; E. M. Leitch; M. Lueker; K. G. Megerian; V. Monticue; T. Namikawa; C. B. Netterfield; H. T. Nguyen; R. O'Brient; R. W. Ogburn; C. Pryke; C. D. Reintsema; S. Richter; R. Schwarz; C. Sorenson; C. D. Sheehy; Z. K. Staniszewski; B. Steinbach; G. P. Teply; K. L. Thompson; J. E. Tolan; C. Tucker; A. D. Turner; A. G. Vieregg; A. Wandui; A. C. Weber; D. V. Wiebe; J. Willmert; W. L.K. Wu; K. W. Yoon

doi:10.1117/12.2233894

BICEP3 performance overview and planned Keck Array upgrade

J. A. Grayson
, P. A.R. Ade
, Z. Ahmed
, K. D. Alexander
, M. Amiri
, D. Barkats
, S. J. Benton
, C. A. Bischoff
, J. J. Bock
, H. Boenish
, R. Bowens-Rubin
, I. Buder
, E. Bullock
, V. Buza
, J. Connors
, J. P. Filippini
, S. Fliescher
, M. Halpern
, S. Harrison
, G. C. Hilton

V. V. Hristov, H. Hui, K. D. Irwin, J. Kang, K. S. Karkare, E. Karpel, S. Kefeli, S. A. Kernasovskiy, J. M. Kovac, C. L. Kuo, E. M. Leitch, M. Lueker, K. G. Megerian, V. Monticue, T. Namikawa, C. B. Netterfield, H. T. Nguyen, R. O'Brient, R. W. Ogburn, C. Pryke, C. D. Reintsema, S. Richter, R. Schwarz, C. Sorenson, C. D. Sheehy, Z. K. Staniszewski, B. Steinbach, G. P. Teply, K. L. Thompson, J. E. Tolan, C. Tucker, A. D. Turner, A. G. Vieregg, A. Wandui, A. C. Weber, D. V. Wiebe, J. Willmert, W. L.K. Wu, K. W. Yoon

Physics

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

58 Scopus citations

Abstract

Bicep3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in Bicep2 and the Keck Array. The increased per-receiver optical throughput compared to Bicep2/Keck Array, due to both its faster f=1:7 optics and the larger aperture, more than doubles the combined mapping speed of the Bicep/Keck program. The Bicep3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, Bicep3- class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Editors	Jonas Zmuidzinas, Wayne S. Holland
Publisher	SPIE
ISBN (Electronic)	9781510602076
DOIs	https://doi.org/10.1117/12.2233894
State	Published - 2016
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII - Edinburgh, United Kingdom Duration: Jun 28 2016 → Jul 1 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9914
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Country/Territory	United Kingdom
City	Edinburgh
Period	6/28/16 → 7/1/16

All Science Journal Classification (ASJC) codes

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

Keywords

BICEP
Cosmic Microwave Background
Gravitational Waves
Inflation
Keck Array
Polarization

Access to Document

10.1117/12.2233894

Cite this

Grayson, J. A., Ade, P. A. R., Ahmed, Z., Alexander, K. D., Amiri, M., Barkats, D., Benton, S. J., Bischoff, C. A., Bock, J. J., Boenish, H., Bowens-Rubin, R., Buder, I., Bullock, E., Buza, V., Connors, J., Filippini, J. P., Fliescher, S., Halpern, M., Harrison, S., ... Yoon, K. W. (2016). BICEP3 performance overview and planned Keck Array upgrade. In J. Zmuidzinas, & W. S. Holland (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII Article 99140S (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9914). SPIE. https://doi.org/10.1117/12.2233894

@inproceedings{df00ca80ec2947448ff105d57ce3e8f1,

title = "BICEP3 performance overview and planned Keck Array upgrade",

abstract = "Bicep3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in Bicep2 and the Keck Array. The increased per-receiver optical throughput compared to Bicep2/Keck Array, due to both its faster f=1:7 optics and the larger aperture, more than doubles the combined mapping speed of the Bicep/Keck program. The Bicep3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, Bicep3- class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new {"}BICEP Array{"} that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.",

keywords = "BICEP, Cosmic Microwave Background, Gravitational Waves, Inflation, Keck Array, Polarization",

author = "Grayson, \{J. A.\} and Ade, \{P. A.R.\} and Z. Ahmed and Alexander, \{K. D.\} and M. Amiri and D. Barkats and Benton, \{S. J.\} and Bischoff, \{C. A.\} and Bock, \{J. J.\} and H. Boenish and R. Bowens-Rubin and I. Buder and E. Bullock and V. Buza and J. Connors and Filippini, \{J. P.\} and S. Fliescher and M. Halpern and S. Harrison and Hilton, \{G. C.\} and Hristov, \{V. V.\} and H. Hui and Irwin, \{K. D.\} and J. Kang and Karkare, \{K. S.\} and E. Karpel and S. Kefeli and Kernasovskiy, \{S. A.\} and Kovac, \{J. M.\} and Kuo, \{C. L.\} and Leitch, \{E. M.\} and M. Lueker and Megerian, \{K. G.\} and V. Monticue and T. Namikawa and Netterfield, \{C. B.\} and Nguyen, \{H. T.\} and R. O'Brient and Ogburn, \{R. W.\} and C. Pryke and Reintsema, \{C. D.\} and S. Richter and R. Schwarz and C. Sorenson and Sheehy, \{C. D.\} and Staniszewski, \{Z. K.\} and B. Steinbach and Teply, \{G. P.\} and Thompson, \{K. L.\} and Tolan, \{J. E.\} and C. Tucker and Turner, \{A. D.\} and Vieregg, \{A. G.\} and A. Wandui and Weber, \{A. C.\} and Wiebe, \{D. V.\} and J. Willmert and Wu, \{W. L.K.\} and Yoon, \{K. W.\}",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII ; Conference date: 28-06-2016 Through 01-07-2016",

year = "2016",

doi = "10.1117/12.2233894",

language = "English (US)",

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

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Holland, \{Wayne S.\}",

booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII",

address = "United States",

}

Grayson, JA, Ade, PAR, Ahmed, Z, Alexander, KD, Amiri, M, Barkats, D, Benton, SJ, Bischoff, CA, Bock, JJ, Boenish, H, Bowens-Rubin, R, Buder, I, Bullock, E, Buza, V, Connors, J, Filippini, JP, Fliescher, S, Halpern, M, Harrison, S, Hilton, GC, Hristov, VV, Hui, H, Irwin, KD, Kang, J, Karkare, KS, Karpel, E, Kefeli, S, Kernasovskiy, SA, Kovac, JM, Kuo, CL, Leitch, EM, Lueker, M, Megerian, KG, Monticue, V, Namikawa, T, Netterfield, CB, Nguyen, HT, O'Brient, R, Ogburn, RW, Pryke, C, Reintsema, CD, Richter, S, Schwarz, R, Sorenson, C, Sheehy, CD, Staniszewski, ZK, Steinbach, B, Teply, GP, Thompson, KL, Tolan, JE, Tucker, C, Turner, AD, Vieregg, AG, Wandui, A, Weber, AC, Wiebe, DV, Willmert, J, Wu, WLK & Yoon, KW 2016, BICEP3 performance overview and planned Keck Array upgrade. in J Zmuidzinas & WS Holland (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII., 99140S, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9914, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, Edinburgh, United Kingdom, 6/28/16. https://doi.org/10.1117/12.2233894

BICEP3 performance overview and planned Keck Array upgrade. / Grayson, J. A.; Ade, P. A.R.; Ahmed, Z. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII. ed. / Jonas Zmuidzinas; Wayne S. Holland. SPIE, 2016. 99140S (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9914).

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

TY - GEN

T1 - BICEP3 performance overview and planned Keck Array upgrade

AU - Grayson, J. A.

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Alexander, K. D.

AU - Amiri, M.

AU - Barkats, D.

AU - Benton, S. J.

AU - Bischoff, C. A.

AU - Bock, J. J.

AU - Boenish, H.

AU - Bowens-Rubin, R.

AU - Buder, I.

AU - Bullock, E.

AU - Buza, V.

AU - Connors, J.

AU - Filippini, J. P.

AU - Fliescher, S.

AU - Halpern, M.

AU - Harrison, S.

AU - Hilton, G. C.

AU - Hristov, V. V.

AU - Hui, H.

AU - Irwin, K. D.

AU - Kang, J.

AU - Karkare, K. S.

AU - Karpel, E.

AU - Kefeli, S.

AU - Kernasovskiy, S. A.

AU - Kovac, J. M.

AU - Kuo, C. L.

AU - Leitch, E. M.

AU - Lueker, M.

AU - Megerian, K. G.

AU - Monticue, V.

AU - Namikawa, T.

AU - Netterfield, C. B.

AU - Nguyen, H. T.

AU - O'Brient, R.

AU - Ogburn, R. W.

AU - Pryke, C.

AU - Reintsema, C. D.

AU - Richter, S.

AU - Schwarz, R.

AU - Sorenson, C.

AU - Sheehy, C. D.

AU - Staniszewski, Z. K.

AU - Steinbach, B.

AU - Teply, G. P.

AU - Thompson, K. L.

AU - Tolan, J. E.

AU - Tucker, C.

AU - Turner, A. D.

AU - Vieregg, A. G.

AU - Wandui, A.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Willmert, J.

AU - Wu, W. L.K.

AU - Yoon, K. W.

PY - 2016

Y1 - 2016

N2 - Bicep3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in Bicep2 and the Keck Array. The increased per-receiver optical throughput compared to Bicep2/Keck Array, due to both its faster f=1:7 optics and the larger aperture, more than doubles the combined mapping speed of the Bicep/Keck program. The Bicep3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, Bicep3- class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.

AB - Bicep3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in Bicep2 and the Keck Array. The increased per-receiver optical throughput compared to Bicep2/Keck Array, due to both its faster f=1:7 optics and the larger aperture, more than doubles the combined mapping speed of the Bicep/Keck program. The Bicep3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, Bicep3- class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.

KW - BICEP

KW - Cosmic Microwave Background

KW - Gravitational Waves

KW - Inflation

KW - Keck Array

KW - Polarization

UR - https://www.scopus.com/pages/publications/85015037971

UR - https://www.scopus.com/pages/publications/85015037971#tab=citedBy

U2 - 10.1117/12.2233894

DO - 10.1117/12.2233894

M3 - Conference contribution

AN - SCOPUS:85015037971

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

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

A2 - Zmuidzinas, Jonas

A2 - Holland, Wayne S.

PB - SPIE

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

Y2 - 28 June 2016 through 1 July 2016

ER -

Grayson JA, Ade PAR, Ahmed Z, Alexander KD, Amiri M, Barkats D et al. BICEP3 performance overview and planned Keck Array upgrade. In Zmuidzinas J, Holland WS, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII. SPIE. 2016. 99140S. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2233894

BICEP3 performance overview and planned Keck Array upgrade

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All Science Journal Classification (ASJC) codes

Keywords

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