BICEP Array cryostat and mount design

Crumrine, Michael, Ade, P. A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Ahmed, Z., Aikin, R. W., Alexander, K. D., Barkats, D., Benton, S. J., Bishchoff, C. A., Bock, J. J., Bowens-Rubin, R., Brevik, J. A., Buder, I., Bullock, E., Buza, V., Connors, J., Cornelison, J., Crill, B. P., Dierickx, M., Duband, L., Dvorkin, C., Filippini, J. P., Filescher, S., Grayson, J. A., Hall, G., Halpern, M., Harrison, S. A., Hildebrandt, S. R., Hilton, G. C., Hui, H., Irwin, K. D., Kang, J. H., Karkare, K. S., Karpel, E., Kaufman, J. P., Keating, B. G., Kefeli, S., Kemasovskiy, S. A., Kovac, J. M., Kuo, C. L., Larsen, N. A., Lau, K., Leitch, E. M., Lueker, M. V., Megerian, K. G., Moncelsi, L., Namikawa, T., Netterfield, C. B., Nguyen, H. T., O'Brient, R., Ogburn IV, R. W., Palladino, S., Pryke, C., Racine, B., Richter, S., Schwarz, R., Schillaci, A., Sheehy, C. D., Soliman, A., St. Germaine, T., Staniszewski, Z. K., Steinbach, B., Sudiwala, R. V. ORCID: https://orcid.org/0000-0003-3240-5304, Teply, G. P., Thompson, K. L., Tolan, J. E., Tucker, C. E. ORCID: https://orcid.org/0000-0002-1851-3918, Turner, A. D., Umilta, C., Vieregg, A. G., Wandui, A., Weber, A. C., Wiebe, D. V., WIllmert, J., Wong, C. L., Wu, W. L. K., Yang, E., Yoon, K. W. and Zhang, C. 2018. BICEP Array cryostat and mount design. Presented at: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, USA, 10-15 June 2018. Proceedings Volume 10708, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. , vol.10708 SPIE, 107082D. 10.1117/12.2312829

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Abstract

Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style receivers that compose the Keck Array with four larger Bicep3 style receivers observing at six frequencies from 30 to 270GHz. The 95GHz and 150GHz receivers will continue to push the already deep Bicep/Keck CMB maps while the 30/40GHz and 220/270GHz receivers will constrain the synchrotron and galactic dust foregrounds respectively. Here we report on the design and performance of the Bicep Array instruments focusing on the mount and cryostat systems....

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Published Online
Status:	Published
Schools:	Physics and Astronomy
Publisher:	SPIE
Last Modified:	27 Apr 2023 15:45
URI:	https://orca.cardiff.ac.uk/id/eprint/156731

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