Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

A. Soliman; P. A.R. Ade; Z. Ahmed; R. W. Aikin; K. D. Alexander; D. Barkats; S. J. Benton; C. A. Bischoff; J. J. Bock; R. Bowens-Rubin; J. A. Brevik; I. Buder; E. Bullock; V. Buza; J. Connors; J. Cornelison; B. P. Crill; M. Crumrine; M. Dierickx; L. Duband; C. Dvorkin; J. P. Filippini; S. Fliescher; J. A. Grayson; G. Hall; M. Halpern; S. Harrison; S. R. Hildebrandt; G. C. Hilton; H. Hui; K. D. Irwin; J. H. Kang; K. S. Karkare; E. Karpel; J. P. Kaufman; B. G. Keating; S. Kefeli; S. A. Kernasovskiy; J. M. Kovac; C. L. Kuo; K. Lau; N. A. Larsen; E. M. Leitch; M. Lueker; K. G. Megerian; L. Moncelsi; T. Namikawa; C. B. Netterfield; H. T. Nguyen; R. O. Brient; R. W. Ogburn; S. Palladino; C. Pryke; B. Racine; S. Richter; R. Schwarz; A. Schillaci; C. D. Sheehy; T. St Germaine; Z. K. Staniszewski; B. Steinbach; R. Sudiwala; G. P. Teply; K. L. Thompson; J. E. Tolan; C. Tucker; A. D. Turner; C. Umiltà; J. Van Zyl; A. G. Vieregg; A. Wandui; A. C. Weber; D. V. Wiebe; J. Willmert; C. L. Wong; W. L.K. Wu; E. Yang; K. W. Yoon; C. Zhang

doi:10.1117/12.2312942

Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

A. Soliman, P. A.R. Ade, Z. Ahmed, R. W. Aikin, K. D. Alexander, D. Barkats, S. J. Benton, C. A. Bischoff, J. J. Bock, R. Bowens-Rubin, J. A. Brevik, I. Buder, E. Bullock, V. Buza, J. Connors, J. Cornelison, B. P. Crill, M. Crumrine, M. Dierickx, L. DubandC. Dvorkin, J. P. Filippini, S. Fliescher, J. A. Grayson, G. Hall, M. Halpern, S. Harrison, S. R. Hildebrandt, G. C. Hilton, H. Hui, K. D. Irwin, J. H. Kang, K. S. Karkare, E. Karpel, J. P. Kaufman, B. G. Keating, S. Kefeli, S. A. Kernasovskiy, J. M. Kovac, C. L. Kuo, K. Lau, N. A. Larsen, E. M. Leitch, M. Lueker, K. G. Megerian, L. Moncelsi, T. Namikawa, C. B. Netterfield, H. T. Nguyen, R. O. Brient, R. W. Ogburn, S. Palladino, C. Pryke, B. Racine, S. Richter, R. Schwarz, A. Schillaci, C. D. Sheehy, T. St Germaine, Z. K. Staniszewski, B. Steinbach, R. Sudiwala, G. P. Teply, K. L. Thompson, J. E. Tolan, C. Tucker, A. D. Turner, C. Umiltà, J. Van Zyl, A. G. Vieregg, A. Wandui, A. C. Weber, D. V. Wiebe, J. Willmert, C. L. Wong, W. L.K. Wu, E. Yang, K. W. Yoon, C. Zhang

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

Abstract

BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single-and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Print)	9781510619692
DOIs	https://doi.org/10.1117/12.2312942
State	Published - 2018
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 - Austin, United States Duration: Jun 12 2018 → Jun 15 2018

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10708
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018
Country/Territory	United States
City	Austin
Period	6/12/18 → 6/15/18

Keywords

BICEP Array
Beam Systematic
Corrugations
Cosmic Microwave Background
Detector

ASJC Scopus subject areas

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

Online availability

10.1117/12.2312942

Library availability

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Soliman, A., Ade, P. A. R., Ahmed, Z., Aikin, R. W., Alexander, K. D., Barkats, D., Benton, S. J., Bischoff, C. A., Bock, J. J., Bowens-Rubin, R., Brevik, J. A., Buder, I., Bullock, E., Buza, V., Connors, J., Cornelison, J., Crill, B. P., Crumrine, M., Dierickx, M., ... Zhang, C. (2018). Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX Article 107082G (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708). SPIE. https://doi.org/10.1117/12.2312942

Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz. / Soliman, A.; Ade, P. A.R.; Ahmed, Z. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2018. 107082G (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708).

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

Soliman, A, Ade, PAR, Ahmed, Z, Aikin, RW, Alexander, KD, Barkats, D, Benton, SJ, Bischoff, CA, Bock, JJ, Bowens-Rubin, R, Brevik, JA, Buder, I, Bullock, E, Buza, V, Connors, J, Cornelison, J, Crill, BP, Crumrine, M, Dierickx, M, Duband, L, Dvorkin, C, Filippini, JP, Fliescher, S, Grayson, JA, Hall, G, Halpern, M, Harrison, S, Hildebrandt, SR, Hilton, GC, Hui, H, Irwin, KD, Kang, JH, Karkare, KS, Karpel, E, Kaufman, JP, Keating, BG, Kefeli, S, Kernasovskiy, SA, Kovac, JM, Kuo, CL, Lau, K, Larsen, NA, Leitch, EM, Lueker, M, Megerian, KG, Moncelsi, L, Namikawa, T, Netterfield, CB, Nguyen, HT, Brient, RO, Ogburn, RW, Palladino, S, Pryke, C, Racine, B, Richter, S, Schwarz, R, Schillaci, A, Sheehy, CD, St Germaine, T, Staniszewski, ZK, Steinbach, B, Sudiwala, R, Teply, GP, Thompson, KL, Tolan, JE, Tucker, C, Turner, AD, Umiltà, C, Van Zyl, J, Vieregg, AG, Wandui, A, Weber, AC, Wiebe, DV, Willmert, J, Wong, CL, Wu, WLK, Yang, E, Yoon, KW & Zhang, C 2018, Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX., 107082G, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10708, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018, Austin, United States, 6/12/18. https://doi.org/10.1117/12.2312942

Soliman A, Ade PAR, Ahmed Z, Aikin RW, Alexander KD, Barkats D et al. Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz. In Zmuidzinas J, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. SPIE. 2018. 107082G. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2312942

Soliman, A. ; Ade, P. A.R. ; Ahmed, Z. et al. / Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz. Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. editor / Jonas Zmuidzinas ; Jian-Rong Gao. SPIE, 2018. (Proceedings of SPIE - The International Society for Optical Engineering).

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title = "Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz",

abstract = "BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single-and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.",

keywords = "BICEP Array, Beam Systematic, Corrugations, Cosmic Microwave Background, Detector",

author = "A. Soliman and Ade, {P. A.R.} and Z. Ahmed and Aikin, {R. W.} and Alexander, {K. D.} and D. Barkats and Benton, {S. J.} and Bischoff, {C. A.} and Bock, {J. J.} and R. Bowens-Rubin and Brevik, {J. A.} and I. Buder and E. Bullock and V. Buza and J. Connors and J. Cornelison and Crill, {B. P.} and M. Crumrine and M. Dierickx and L. Duband and C. Dvorkin and Filippini, {J. P.} and S. Fliescher and Grayson, {J. A.} and G. Hall and M. Halpern and S. Harrison and Hildebrandt, {S. R.} and Hilton, {G. C.} and H. Hui and Irwin, {K. D.} and Kang, {J. H.} and Karkare, {K. S.} and E. Karpel and Kaufman, {J. P.} and Keating, {B. G.} and S. Kefeli and Kernasovskiy, {S. A.} and Kovac, {J. M.} and Kuo, {C. L.} and K. Lau and Larsen, {N. A.} and Leitch, {E. M.} and M. Lueker and Megerian, {K. G.} and L. Moncelsi and T. Namikawa and Netterfield, {C. B.} and Nguyen, {H. T.} and Brient, {R. O.} and Ogburn, {R. W.} and S. Palladino and C. Pryke and B. Racine and S. Richter and R. Schwarz and A. Schillaci and Sheehy, {C. D.} and {St Germaine}, T. and Staniszewski, {Z. K.} and B. Steinbach and R. Sudiwala and Teply, {G. P.} and Thompson, {K. L.} and Tolan, {J. E.} and C. Tucker and Turner, {A. D.} and C. Umilt{\`a} and {Van Zyl}, J. and Vieregg, {A. G.} and A. Wandui and Weber, {A. C.} and Wiebe, {D. V.} and J. Willmert and Wong, {C. L.} and Wu, {W. L.K.} and E. Yang and Yoon, {K. W.} and C. Zhang",

note = "Publisher Copyright: {\textcopyright} 2018 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 ; Conference date: 12-06-2018 Through 15-06-2018",

year = "2018",

doi = "10.1117/12.2312942",

language = "English (US)",

isbn = "9781510619692",

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

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao",

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

}

TY - GEN

T1 - Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

AU - Soliman, A.

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Aikin, R. W.

AU - Alexander, K. D.

AU - Barkats, D.

AU - Benton, S. J.

AU - Bischoff, C. A.

AU - Bock, J. J.

AU - Bowens-Rubin, R.

AU - Brevik, J. A.

AU - Buder, I.

AU - Bullock, E.

AU - Buza, V.

AU - Connors, J.

AU - Cornelison, J.

AU - Crill, B. P.

AU - Crumrine, M.

AU - Dierickx, M.

AU - Duband, L.

AU - Dvorkin, C.

AU - Filippini, J. P.

AU - Fliescher, S.

AU - Grayson, J. A.

AU - Hall, G.

AU - Halpern, M.

AU - Harrison, S.

AU - Hildebrandt, S. R.

AU - Hilton, G. C.

AU - Hui, H.

AU - Irwin, K. D.

AU - Kang, J. H.

AU - Karkare, K. S.

AU - Karpel, E.

AU - Kaufman, J. P.

AU - Keating, B. G.

AU - Kefeli, S.

AU - Kernasovskiy, S. A.

AU - Kovac, J. M.

AU - Kuo, C. L.

AU - Lau, K.

AU - Larsen, N. A.

AU - Leitch, E. M.

AU - Lueker, M.

AU - Megerian, K. G.

AU - Moncelsi, L.

AU - Namikawa, T.

AU - Netterfield, C. B.

AU - Nguyen, H. T.

AU - Brient, R. O.

AU - Ogburn, R. W.

AU - Palladino, S.

AU - Pryke, C.

AU - Racine, B.

AU - Richter, S.

AU - Schwarz, R.

AU - Schillaci, A.

AU - Sheehy, C. D.

AU - St Germaine, T.

AU - Staniszewski, Z. K.

AU - Steinbach, B.

AU - Sudiwala, R.

AU - Teply, G. P.

AU - Thompson, K. L.

AU - Tolan, J. E.

AU - Tucker, C.

AU - Turner, A. D.

AU - Umiltà, C.

AU - Van Zyl, J.

AU - Vieregg, A. G.

AU - Wandui, A.

AU - Weber, A. C.

AU - Wiebe, D. V.

AU - Willmert, J.

AU - Wong, C. L.

AU - Wu, W. L.K.

AU - Yang, E.

AU - Yoon, K. W.

AU - Zhang, C.

PY - 2018

Y1 - 2018

N2 - BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single-and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.

AB - BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single-and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.

KW - BICEP Array

KW - Beam Systematic

KW - Corrugations

KW - Cosmic Microwave Background

KW - Detector

UR - http://www.scopus.com/inward/record.url?scp=85051983712&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85051983712&partnerID=8YFLogxK

U2 - 10.1117/12.2312942

DO - 10.1117/12.2312942

M3 - Conference contribution

AN - SCOPUS:85051983712

SN - 9781510619692

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

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

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018

Y2 - 12 June 2018 through 15 June 2018

ER -

Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

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