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Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers

Fuente: arXiv

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Main Authors:	Fatigoni, S., Ade, P. A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, Bischoff, C. A., Beck, D., Bock, J. J., Buza, V., Cheshire, J., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A. J., Denison, E. V., Dierickx, M. I., Duband, L., Eiben, M., Filippini, J. P., Fortes, A., Gao, M., Giannakopoulos, C., Goeckner-Wald, N., Goldfinger, D. C., Grayson, J. A., Grimes, P. K., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S. A., Handerson, S., Hildebrandt, S. R., Hilton, G. C., Hubmayr, J., Hui, H., Irwin, K. D., Kang, J. H., Karkare, K. S., Kefeli, S., Kovac, J. M., Kuo, C. L., Lau, K., Lennox, A., Liu, T., Megerian, K. G., Miller, O. Y., Minutolo, L., Moncelsi, L., Nakato, Y., Nguyen, H. T., Brient, R. O, Palladino, S., Petroff, M. A., Polish, A., Prouve, T., Pryke, C., Racine, B., Reintsema, C. D., Romand, T., Salatino, M., Schillaci, A., Schmitt, B. L., Singari, B., Soliman, A., Germaine, T. St., Steiger, A., Steinbach, B., Sudiwala, R., Thompson, K. L., Tsai, C., Tucker, C., Turner, A. D., Umiltà, C., Vèrges, C., Wandui, A., Weber, A. C., Wiebe, D. V., Willmert, J., Wu, W. L. K., Yang, E., Young, E., Yu, C., Zeng, L., Zhang, C., Zhang, S.
Format:	Preprint
Published:	2023
Subjects:	Instrumentation and Methods for Astrophysics Instrumentation and Detectors
Online Access:	Acceder al recurso
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author	Fatigoni, S. Ade, P. A. R. Ahmed, Z. Amiri, M. Barkats, D. Thakur, R. Basu Bischoff, C. A. Beck, D. Bock, J. J. Buza, V. Cheshire, J. Connors, J. Cornelison, J. Crumrine, M. Cukierman, A. J. Denison, E. V. Dierickx, M. I. Duband, L. Eiben, M. Filippini, J. P. Fortes, A. Gao, M. Giannakopoulos, C. Goeckner-Wald, N. Goldfinger, D. C. Grayson, J. A. Grimes, P. K. Hall, G. Halal, G. Halpern, M. Hand, E. Harrison, S. A. Handerson, S. Hildebrandt, S. R. Hilton, G. C. Hubmayr, J. Hui, H. Irwin, K. D. Kang, J. H. Karkare, K. S. Kefeli, S. Kovac, J. M. Kuo, C. L. Lau, K. Lennox, A. Liu, T. Megerian, K. G. Miller, O. Y. Minutolo, L. Moncelsi, L. Nakato, Y. Nguyen, H. T. Brient, R. O Palladino, S. Petroff, M. A. Polish, A. Prouve, T. Pryke, C. Racine, B. Reintsema, C. D. Romand, T. Salatino, M. Schillaci, A. Schmitt, B. L. Singari, B. Soliman, A. Germaine, T. St. Steiger, A. Steinbach, B. Sudiwala, R. Thompson, K. L. Tsai, C. Tucker, C. Turner, A. D. Umiltà, C. Vèrges, C. Wandui, A. Weber, A. C. Wiebe, D. V. Willmert, J. Wu, W. L. K. Yang, E. Young, E. Yu, C. Zeng, L. Zhang, C. Zhang, S.
author_facet	Fatigoni, S. Ade, P. A. R. Ahmed, Z. Amiri, M. Barkats, D. Thakur, R. Basu Bischoff, C. A. Beck, D. Bock, J. J. Buza, V. Cheshire, J. Connors, J. Cornelison, J. Crumrine, M. Cukierman, A. J. Denison, E. V. Dierickx, M. I. Duband, L. Eiben, M. Filippini, J. P. Fortes, A. Gao, M. Giannakopoulos, C. Goeckner-Wald, N. Goldfinger, D. C. Grayson, J. A. Grimes, P. K. Hall, G. Halal, G. Halpern, M. Hand, E. Harrison, S. A. Handerson, S. Hildebrandt, S. R. Hilton, G. C. Hubmayr, J. Hui, H. Irwin, K. D. Kang, J. H. Karkare, K. S. Kefeli, S. Kovac, J. M. Kuo, C. L. Lau, K. Lennox, A. Liu, T. Megerian, K. G. Miller, O. Y. Minutolo, L. Moncelsi, L. Nakato, Y. Nguyen, H. T. Brient, R. O Palladino, S. Petroff, M. A. Polish, A. Prouve, T. Pryke, C. Racine, B. Reintsema, C. D. Romand, T. Salatino, M. Schillaci, A. Schmitt, B. L. Singari, B. Soliman, A. Germaine, T. St. Steiger, A. Steinbach, B. Sudiwala, R. Thompson, K. L. Tsai, C. Tucker, C. Turner, A. D. Umiltà, C. Vèrges, C. Wandui, A. Weber, A. C. Wiebe, D. V. Willmert, J. Wu, W. L. K. Yang, E. Young, E. Yu, C. Zeng, L. Zhang, C. Zhang, S.
contents	Time-Division Multiplexing is the readout architecture of choice for many ground and space experiments, as it is a very mature technology with proven outstanding low-frequency noise stability, which represents a central challenge in multiplexing. Once fully populated, each of the two BICEP Array high frequency receivers, observing at 150GHz and 220/270GHz, will have 7776 TES detectors tiled on the focal plane. The constraints set by these two receivers required a redesign of the warm readout electronics. The new version of the standard Multi Channel Electronics, developed and built at the University of British Columbia, is presented here for the first time. BICEP Array operates Time Division Multiplexing readout technology to the limits of its capabilities in terms of multiplexing rate, noise and crosstalk, and applies them in rigorously demanding scientific application requiring extreme noise performance and systematic error control. Future experiments like CMB-S4 plan to use TES bolometers with Time Division/SQUID-based readout for an even larger number of detectors.
format	Preprint
id	arxiv_https___arxiv_org_abs_2310_10849
institution	arXiv
publishDate	2023
record_format	arxiv
spellingShingle	Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers Fatigoni, S. Ade, P. A. R. Ahmed, Z. Amiri, M. Barkats, D. Thakur, R. Basu Bischoff, C. A. Beck, D. Bock, J. J. Buza, V. Cheshire, J. Connors, J. Cornelison, J. Crumrine, M. Cukierman, A. J. Denison, E. V. Dierickx, M. I. Duband, L. Eiben, M. Filippini, J. P. Fortes, A. Gao, M. Giannakopoulos, C. Goeckner-Wald, N. Goldfinger, D. C. Grayson, J. A. Grimes, P. K. Hall, G. Halal, G. Halpern, M. Hand, E. Harrison, S. A. Handerson, S. Hildebrandt, S. R. Hilton, G. C. Hubmayr, J. Hui, H. Irwin, K. D. Kang, J. H. Karkare, K. S. Kefeli, S. Kovac, J. M. Kuo, C. L. Lau, K. Lennox, A. Liu, T. Megerian, K. G. Miller, O. Y. Minutolo, L. Moncelsi, L. Nakato, Y. Nguyen, H. T. Brient, R. O Palladino, S. Petroff, M. A. Polish, A. Prouve, T. Pryke, C. Racine, B. Reintsema, C. D. Romand, T. Salatino, M. Schillaci, A. Schmitt, B. L. Singari, B. Soliman, A. Germaine, T. St. Steiger, A. Steinbach, B. Sudiwala, R. Thompson, K. L. Tsai, C. Tucker, C. Turner, A. D. Umiltà, C. Vèrges, C. Wandui, A. Weber, A. C. Wiebe, D. V. Willmert, J. Wu, W. L. K. Yang, E. Young, E. Yu, C. Zeng, L. Zhang, C. Zhang, S. Instrumentation and Methods for Astrophysics Instrumentation and Detectors Time-Division Multiplexing is the readout architecture of choice for many ground and space experiments, as it is a very mature technology with proven outstanding low-frequency noise stability, which represents a central challenge in multiplexing. Once fully populated, each of the two BICEP Array high frequency receivers, observing at 150GHz and 220/270GHz, will have 7776 TES detectors tiled on the focal plane. The constraints set by these two receivers required a redesign of the warm readout electronics. The new version of the standard Multi Channel Electronics, developed and built at the University of British Columbia, is presented here for the first time. BICEP Array operates Time Division Multiplexing readout technology to the limits of its capabilities in terms of multiplexing rate, noise and crosstalk, and applies them in rigorously demanding scientific application requiring extreme noise performance and systematic error control. Future experiments like CMB-S4 plan to use TES bolometers with Time Division/SQUID-based readout for an even larger number of detectors.
title	Results and Limits of Time Division Multiplexing for the BICEP Array High Frequency Receivers
topic	Instrumentation and Methods for Astrophysics Instrumentation and Detectors
url	https://arxiv.org/abs/2310.10849