Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole
A detection of curl-type (B-mode) polarization of the primary CMB would be direct evidence for the inflationary paradigm of the origin of the Universe. The Bicep/Keck Array (BK) program targets the degree angular scales, where the power from primordial B-mode polarization is expected to peak, with e...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | , |
Format: | Book Part |
Language: | English |
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Society of Photo-Optical Instrumentation Engineers (SPIE)
2020
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Subjects: | |
Online Access: | https://authors.library.caltech.edu/107183/ https://authors.library.caltech.edu/107183/1/1145314.pdf https://authors.library.caltech.edu/107183/3/2012.04047.pdf https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299 |
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Caltech Authors (California Institute of Technology) |
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English |
description |
A detection of curl-type (B-mode) polarization of the primary CMB would be direct evidence for the inflationary paradigm of the origin of the Universe. The Bicep/Keck Array (BK) program targets the degree angular scales, where the power from primordial B-mode polarization is expected to peak, with ever-increasing sensitivity and has published the most stringent constraints on inflation to date. Bicep Array (BA) is the Stage-3 instrument of the BK program and will comprise four Bicep3-class receivers observing at 30/40, 95, 150 and 220/270 GHz with a combined 32,000+ detectors; such wide frequency coverage is necessary for control of the Galactic foregrounds, which also produce degree-scale B-mode signal. The 30/40 GHz receiver is designed to constrain the synchrotron foreground and has begun observing at the South Pole in early 2020. By the end of a 3-year observing campaign, the full Bicep Array instrument is projected to reach σr between 0.002 and 0.004, depending on foreground complexity and degree of removal of B-modes due to gravitational lensing (delensing). This paper presents an overview of the design, measured on-sky performance and calibration of the first BA receiver. We also give a preview of the added complexity in the time-domain multiplexed readout of the 7,776-detector 150 GHz receiver. |
author2 |
Zmuidzinas, Jonas Gao, Jian-Rong |
format |
Book Part |
author |
Moncelsi, L. Ade, Peter A. Ahmed, Zeeshan Amiri, Mandana Barkats, Denis Thakur, R. Basu Bischoff, Colin A. Bock, J. J. Buza, Victor Cheshire, James R. Connors, Jake Cornelison, James Crumrine, Michael Cukierman, Ari J. Denison, Edward Dierickx, Marion Duband, Lionel Eiben, Miranda Fatigoni, Sofia Filippini, Jeffrey P. Goeckner-Wald, Neil Goldfinger, David Grayson, James A. Grimes, Paul Hall, Grantland Halpern, Mark Harrison, Samuel A. Henderson, Shawn Hildebrandt, S. R. Hilton, Gene Hubmayr, Johannes Hui, H. Irwin, Kent D. Kang, J. H. Karkare, Kirit S. Kefeli, S. Kovac, John M. Kuo, Chao-Lin Lau, Kenny Leitch, Erik M. Megerian, K. G. Minutolo, L. Nakato, Yuka Namikawa, Toshiya Nguyen, H. T. O'Brient, R. Palladino, Steven Precup, Nathan Prouve, Thomas Pryke, Clement Racine, Benjamin Reintsema, Carl D. Schillaci, A. Schmitt, Benjamin Soliman, A. St. Germaine, Tyler Steinbach, B. Sudiwala, Rashmi Thompson, Keith L. Tucker, Carole Turner, Anthony D. Umiltà, Caterina Vieregg, Abigail G. Wandui, A. Weber, A. C. Wiebe, Don V. Willmert, Justin Wu, Wai Ling K. Yang, Hung-I E. Yoon, Ki Won Young, Edward Y. Yu, Cyndia Zeng, Lingzhen Zhang, C. Zhang, S. |
spellingShingle |
Moncelsi, L. Ade, Peter A. Ahmed, Zeeshan Amiri, Mandana Barkats, Denis Thakur, R. Basu Bischoff, Colin A. Bock, J. J. Buza, Victor Cheshire, James R. Connors, Jake Cornelison, James Crumrine, Michael Cukierman, Ari J. Denison, Edward Dierickx, Marion Duband, Lionel Eiben, Miranda Fatigoni, Sofia Filippini, Jeffrey P. Goeckner-Wald, Neil Goldfinger, David Grayson, James A. Grimes, Paul Hall, Grantland Halpern, Mark Harrison, Samuel A. Henderson, Shawn Hildebrandt, S. R. Hilton, Gene Hubmayr, Johannes Hui, H. Irwin, Kent D. Kang, J. H. Karkare, Kirit S. Kefeli, S. Kovac, John M. Kuo, Chao-Lin Lau, Kenny Leitch, Erik M. Megerian, K. G. Minutolo, L. Nakato, Yuka Namikawa, Toshiya Nguyen, H. T. O'Brient, R. Palladino, Steven Precup, Nathan Prouve, Thomas Pryke, Clement Racine, Benjamin Reintsema, Carl D. Schillaci, A. Schmitt, Benjamin Soliman, A. St. Germaine, Tyler Steinbach, B. Sudiwala, Rashmi Thompson, Keith L. Tucker, Carole Turner, Anthony D. Umiltà, Caterina Vieregg, Abigail G. Wandui, A. Weber, A. C. Wiebe, Don V. Willmert, Justin Wu, Wai Ling K. Yang, Hung-I E. Yoon, Ki Won Young, Edward Y. Yu, Cyndia Zeng, Lingzhen Zhang, C. Zhang, S. Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
author_facet |
Moncelsi, L. Ade, Peter A. Ahmed, Zeeshan Amiri, Mandana Barkats, Denis Thakur, R. Basu Bischoff, Colin A. Bock, J. J. Buza, Victor Cheshire, James R. Connors, Jake Cornelison, James Crumrine, Michael Cukierman, Ari J. Denison, Edward Dierickx, Marion Duband, Lionel Eiben, Miranda Fatigoni, Sofia Filippini, Jeffrey P. Goeckner-Wald, Neil Goldfinger, David Grayson, James A. Grimes, Paul Hall, Grantland Halpern, Mark Harrison, Samuel A. Henderson, Shawn Hildebrandt, S. R. Hilton, Gene Hubmayr, Johannes Hui, H. Irwin, Kent D. Kang, J. H. Karkare, Kirit S. Kefeli, S. Kovac, John M. Kuo, Chao-Lin Lau, Kenny Leitch, Erik M. Megerian, K. G. Minutolo, L. Nakato, Yuka Namikawa, Toshiya Nguyen, H. T. O'Brient, R. Palladino, Steven Precup, Nathan Prouve, Thomas Pryke, Clement Racine, Benjamin Reintsema, Carl D. Schillaci, A. Schmitt, Benjamin Soliman, A. St. Germaine, Tyler Steinbach, B. Sudiwala, Rashmi Thompson, Keith L. Tucker, Carole Turner, Anthony D. Umiltà, Caterina Vieregg, Abigail G. Wandui, A. Weber, A. C. Wiebe, Don V. Willmert, Justin Wu, Wai Ling K. Yang, Hung-I E. Yoon, Ki Won Young, Edward Y. Yu, Cyndia Zeng, Lingzhen Zhang, C. Zhang, S. |
author_sort |
Moncelsi, L. |
title |
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
title_short |
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
title_full |
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
title_fullStr |
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
title_full_unstemmed |
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole |
title_sort |
receiver development for bicep array, a next-generation cmb polarimeter at the south pole |
publisher |
Society of Photo-Optical Instrumentation Engineers (SPIE) |
publishDate |
2020 |
url |
https://authors.library.caltech.edu/107183/ https://authors.library.caltech.edu/107183/1/1145314.pdf https://authors.library.caltech.edu/107183/3/2012.04047.pdf https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299 |
long_lat |
ENVELOPE(-63.071,-63.071,-70.797,-70.797) |
geographic |
Curl South Pole |
geographic_facet |
Curl South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://authors.library.caltech.edu/107183/1/1145314.pdf https://authors.library.caltech.edu/107183/3/2012.04047.pdf Moncelsi, L. and Ade, Peter A. and Ahmed, Zeeshan and Amiri, Mandana and Barkats, Denis and Thakur, R. Basu and Bischoff, Colin A. and Bock, J. J. and Buza, Victor and Cheshire, James R. and Connors, Jake and Cornelison, James and Crumrine, Michael and Cukierman, Ari J. and Denison, Edward and Dierickx, Marion and Duband, Lionel and Eiben, Miranda and Fatigoni, Sofia and Filippini, Jeffrey P. and Goeckner-Wald, Neil and Goldfinger, David and Grayson, James A. and Grimes, Paul and Hall, Grantland and Halpern, Mark and Harrison, Samuel A. and Henderson, Shawn and Hildebrandt, S. R. and Hilton, Gene and Hubmayr, Johannes and Hui, H. and Irwin, Kent D. and Kang, J. H. and Karkare, Kirit S. and Kefeli, S. and Kovac, John M. and Kuo, Chao-Lin and Lau, Kenny and Leitch, Erik M. and Megerian, K. G. and Minutolo, L. and Nakato, Yuka and Namikawa, Toshiya and Nguyen, H. T. and O'Brient, R. and Palladino, Steven and Precup, Nathan and Prouve, Thomas and Pryke, Clement and Racine, Benjamin and Reintsema, Carl D. and Schillaci, A. and Schmitt, Benjamin and Soliman, A. and St. Germaine, Tyler and Steinbach, B. and Sudiwala, Rashmi and Thompson, Keith L. and Tucker, Carole and Turner, Anthony D. and Umiltà, Caterina and Vieregg, Abigail G. and Wandui, A. and Weber, A. C. and Wiebe, Don V. and Willmert, Justin and Wu, Wai Ling K. and Yang, Hung-I E. and Yoon, Ki Won and Young, Edward Y. and Yu, Cyndia and Zeng, Lingzhen and Zhang, C. and Zhang, S. (2020) Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole. In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. Proceedings of SPIE. No.11453. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 1145314. ISBN 9781510636934. https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299 <https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299> |
op_rights |
other |
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1766201447370719232 |
spelling |
ftcaltechauth:oai:authors.library.caltech.edu:107183 2023-05-15T18:22:05+02:00 Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole Moncelsi, L. Ade, Peter A. Ahmed, Zeeshan Amiri, Mandana Barkats, Denis Thakur, R. Basu Bischoff, Colin A. Bock, J. J. Buza, Victor Cheshire, James R. Connors, Jake Cornelison, James Crumrine, Michael Cukierman, Ari J. Denison, Edward Dierickx, Marion Duband, Lionel Eiben, Miranda Fatigoni, Sofia Filippini, Jeffrey P. Goeckner-Wald, Neil Goldfinger, David Grayson, James A. Grimes, Paul Hall, Grantland Halpern, Mark Harrison, Samuel A. Henderson, Shawn Hildebrandt, S. R. Hilton, Gene Hubmayr, Johannes Hui, H. Irwin, Kent D. Kang, J. H. Karkare, Kirit S. Kefeli, S. Kovac, John M. Kuo, Chao-Lin Lau, Kenny Leitch, Erik M. Megerian, K. G. Minutolo, L. Nakato, Yuka Namikawa, Toshiya Nguyen, H. T. O'Brient, R. Palladino, Steven Precup, Nathan Prouve, Thomas Pryke, Clement Racine, Benjamin Reintsema, Carl D. Schillaci, A. Schmitt, Benjamin Soliman, A. St. Germaine, Tyler Steinbach, B. Sudiwala, Rashmi Thompson, Keith L. Tucker, Carole Turner, Anthony D. Umiltà, Caterina Vieregg, Abigail G. Wandui, A. Weber, A. C. Wiebe, Don V. Willmert, Justin Wu, Wai Ling K. Yang, Hung-I E. Yoon, Ki Won Young, Edward Y. Yu, Cyndia Zeng, Lingzhen Zhang, C. Zhang, S. Zmuidzinas, Jonas Gao, Jian-Rong 2020-12-13 application/pdf https://authors.library.caltech.edu/107183/ https://authors.library.caltech.edu/107183/1/1145314.pdf https://authors.library.caltech.edu/107183/3/2012.04047.pdf https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299 en eng Society of Photo-Optical Instrumentation Engineers (SPIE) https://authors.library.caltech.edu/107183/1/1145314.pdf https://authors.library.caltech.edu/107183/3/2012.04047.pdf Moncelsi, L. and Ade, Peter A. and Ahmed, Zeeshan and Amiri, Mandana and Barkats, Denis and Thakur, R. Basu and Bischoff, Colin A. and Bock, J. J. and Buza, Victor and Cheshire, James R. and Connors, Jake and Cornelison, James and Crumrine, Michael and Cukierman, Ari J. and Denison, Edward and Dierickx, Marion and Duband, Lionel and Eiben, Miranda and Fatigoni, Sofia and Filippini, Jeffrey P. and Goeckner-Wald, Neil and Goldfinger, David and Grayson, James A. and Grimes, Paul and Hall, Grantland and Halpern, Mark and Harrison, Samuel A. and Henderson, Shawn and Hildebrandt, S. R. and Hilton, Gene and Hubmayr, Johannes and Hui, H. and Irwin, Kent D. and Kang, J. H. and Karkare, Kirit S. and Kefeli, S. and Kovac, John M. and Kuo, Chao-Lin and Lau, Kenny and Leitch, Erik M. and Megerian, K. G. and Minutolo, L. and Nakato, Yuka and Namikawa, Toshiya and Nguyen, H. T. and O'Brient, R. and Palladino, Steven and Precup, Nathan and Prouve, Thomas and Pryke, Clement and Racine, Benjamin and Reintsema, Carl D. and Schillaci, A. and Schmitt, Benjamin and Soliman, A. and St. Germaine, Tyler and Steinbach, B. and Sudiwala, Rashmi and Thompson, Keith L. and Tucker, Carole and Turner, Anthony D. and Umiltà, Caterina and Vieregg, Abigail G. and Wandui, A. and Weber, A. C. and Wiebe, Don V. and Willmert, Justin and Wu, Wai Ling K. and Yang, Hung-I E. and Yoon, Ki Won and Young, Edward Y. and Yu, Cyndia and Zeng, Lingzhen and Zhang, C. and Zhang, S. (2020) Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole. In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. Proceedings of SPIE. No.11453. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 1145314. ISBN 9781510636934. https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299 <https://resolver.caltech.edu/CaltechAUTHORS:20201218-074706299> other Book Section PeerReviewed 2020 ftcaltechauth 2021-11-18T19:02:37Z A detection of curl-type (B-mode) polarization of the primary CMB would be direct evidence for the inflationary paradigm of the origin of the Universe. The Bicep/Keck Array (BK) program targets the degree angular scales, where the power from primordial B-mode polarization is expected to peak, with ever-increasing sensitivity and has published the most stringent constraints on inflation to date. Bicep Array (BA) is the Stage-3 instrument of the BK program and will comprise four Bicep3-class receivers observing at 30/40, 95, 150 and 220/270 GHz with a combined 32,000+ detectors; such wide frequency coverage is necessary for control of the Galactic foregrounds, which also produce degree-scale B-mode signal. The 30/40 GHz receiver is designed to constrain the synchrotron foreground and has begun observing at the South Pole in early 2020. By the end of a 3-year observing campaign, the full Bicep Array instrument is projected to reach σr between 0.002 and 0.004, depending on foreground complexity and degree of removal of B-modes due to gravitational lensing (delensing). This paper presents an overview of the design, measured on-sky performance and calibration of the first BA receiver. We also give a preview of the added complexity in the time-domain multiplexed readout of the 7,776-detector 150 GHz receiver. Book Part South pole Caltech Authors (California Institute of Technology) Curl ENVELOPE(-63.071,-63.071,-70.797,-70.797) South Pole |