BICEP Array cryostat and mount design

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 2...

Full description

Bibliographic Details
Main Authors: Crumrine, M., Ade, P. A. R., Ahmed, Z., Aikin, R. W., Alexander, K. D., Barkats, D., Benton, S. J., Bischof, 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., Fliescher, S., Grayson, J., Hall, G., Halpern, M., Harrison, S., Hildebrandt, S. R., Hilton, G. C., Hui, H., Irwin, K. D., Kang, J., Karkare, K. S., Karpel, E., Kaufman, J. P., Keating, B. G., Kefeli, S., Kernasovskiy, S. A., Kovac, J. M., Kuo, C. L., Lau, K., Larsen, N. A., Leitch, E. M., Lueker, M., Megerian, K. G., Moncelsi, L., Namikawa, T., Nguyen, H. T., O'Brient, R., Ogburn, R. W., Palladino, S., Pryke, C., Racine, B., Richter, S., Schwarz, R., Schillaci, A., Sheehy, C. D., Soliman, A., Germaine, T. St., Staniszewski, Z. K., Steinbach, B., Sudiwala, R. V., Teply, G. P., Thompson, K. L., Tolan, J. E., Tucker, C., 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, H., Yoon, K. W., Zhang, C.
Format: Report
Language:unknown
Published: arXiv 2018
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1808.00569
https://arxiv.org/abs/1808.00569
id ftdatacite:10.48550/arxiv.1808.00569
record_format openpolar
spelling ftdatacite:10.48550/arxiv.1808.00569 2023-05-15T18:22:24+02:00 BICEP Array cryostat and mount design Crumrine, M. Ade, P. A. R. Ahmed, Z. Aikin, R. W. Alexander, K. D. Barkats, D. Benton, S. J. Bischof, 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. Fliescher, S. Grayson, J. Hall, G. Halpern, M. Harrison, S. Hildebrandt, S. R. Hilton, G. C. Hui, H. Irwin, K. D. Kang, J. Karkare, K. S. Karpel, E. Kaufman, J. P. Keating, B. G. Kefeli, S. Kernasovskiy, S. A. Kovac, J. M. Kuo, C. L. Lau, K. Larsen, N. A. Leitch, E. M. Lueker, M. Megerian, K. G. Moncelsi, L. Namikawa, T. Nguyen, H. T. O'Brient, R. Ogburn, R. W. Palladino, S. Pryke, C. Racine, B. Richter, S. Schwarz, R. Schillaci, A. Sheehy, C. D. Soliman, A. Germaine, T. St. Staniszewski, Z. K. Steinbach, B. Sudiwala, R. V. Teply, G. P. Thompson, K. L. Tolan, J. E. Tucker, C. 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, H. Yoon, K. W. Zhang, C. 2018 https://dx.doi.org/10.48550/arxiv.1808.00569 https://arxiv.org/abs/1808.00569 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Instrumentation and Methods for Astrophysics astro-ph.IM Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Preprint Article article CreativeWork 2018 ftdatacite https://doi.org/10.48550/arxiv.1808.00569 2022-04-01T09:05:24Z 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. : 10 pages, 7 figures. Published in Proc. SPIE. Presented at SPIE Astronomical Telescopes and Instrumentation Conference 10708: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, June 2018 Report South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Instrumentation and Methods for Astrophysics astro-ph.IM
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
spellingShingle Instrumentation and Methods for Astrophysics astro-ph.IM
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
Crumrine, M.
Ade, P. A. R.
Ahmed, Z.
Aikin, R. W.
Alexander, K. D.
Barkats, D.
Benton, S. J.
Bischof, 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.
Fliescher, S.
Grayson, J.
Hall, G.
Halpern, M.
Harrison, S.
Hildebrandt, S. R.
Hilton, G. C.
Hui, H.
Irwin, K. D.
Kang, J.
Karkare, K. S.
Karpel, E.
Kaufman, J. P.
Keating, B. G.
Kefeli, S.
Kernasovskiy, S. A.
Kovac, J. M.
Kuo, C. L.
Lau, K.
Larsen, N. A.
Leitch, E. M.
Lueker, M.
Megerian, K. G.
Moncelsi, L.
Namikawa, T.
Nguyen, H. T.
O'Brient, R.
Ogburn, R. W.
Palladino, S.
Pryke, C.
Racine, B.
Richter, S.
Schwarz, R.
Schillaci, A.
Sheehy, C. D.
Soliman, A.
Germaine, T. St.
Staniszewski, Z. K.
Steinbach, B.
Sudiwala, R. V.
Teply, G. P.
Thompson, K. L.
Tolan, J. E.
Tucker, C.
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, H.
Yoon, K. W.
Zhang, C.
BICEP Array cryostat and mount design
topic_facet Instrumentation and Methods for Astrophysics astro-ph.IM
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
description 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. : 10 pages, 7 figures. Published in Proc. SPIE. Presented at SPIE Astronomical Telescopes and Instrumentation Conference 10708: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, June 2018
format Report
author Crumrine, M.
Ade, P. A. R.
Ahmed, Z.
Aikin, R. W.
Alexander, K. D.
Barkats, D.
Benton, S. J.
Bischof, 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.
Fliescher, S.
Grayson, J.
Hall, G.
Halpern, M.
Harrison, S.
Hildebrandt, S. R.
Hilton, G. C.
Hui, H.
Irwin, K. D.
Kang, J.
Karkare, K. S.
Karpel, E.
Kaufman, J. P.
Keating, B. G.
Kefeli, S.
Kernasovskiy, S. A.
Kovac, J. M.
Kuo, C. L.
Lau, K.
Larsen, N. A.
Leitch, E. M.
Lueker, M.
Megerian, K. G.
Moncelsi, L.
Namikawa, T.
Nguyen, H. T.
O'Brient, R.
Ogburn, R. W.
Palladino, S.
Pryke, C.
Racine, B.
Richter, S.
Schwarz, R.
Schillaci, A.
Sheehy, C. D.
Soliman, A.
Germaine, T. St.
Staniszewski, Z. K.
Steinbach, B.
Sudiwala, R. V.
Teply, G. P.
Thompson, K. L.
Tolan, J. E.
Tucker, C.
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, H.
Yoon, K. W.
Zhang, C.
author_facet Crumrine, M.
Ade, P. A. R.
Ahmed, Z.
Aikin, R. W.
Alexander, K. D.
Barkats, D.
Benton, S. J.
Bischof, 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.
Fliescher, S.
Grayson, J.
Hall, G.
Halpern, M.
Harrison, S.
Hildebrandt, S. R.
Hilton, G. C.
Hui, H.
Irwin, K. D.
Kang, J.
Karkare, K. S.
Karpel, E.
Kaufman, J. P.
Keating, B. G.
Kefeli, S.
Kernasovskiy, S. A.
Kovac, J. M.
Kuo, C. L.
Lau, K.
Larsen, N. A.
Leitch, E. M.
Lueker, M.
Megerian, K. G.
Moncelsi, L.
Namikawa, T.
Nguyen, H. T.
O'Brient, R.
Ogburn, R. W.
Palladino, S.
Pryke, C.
Racine, B.
Richter, S.
Schwarz, R.
Schillaci, A.
Sheehy, C. D.
Soliman, A.
Germaine, T. St.
Staniszewski, Z. K.
Steinbach, B.
Sudiwala, R. V.
Teply, G. P.
Thompson, K. L.
Tolan, J. E.
Tucker, C.
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, H.
Yoon, K. W.
Zhang, C.
author_sort Crumrine, M.
title BICEP Array cryostat and mount design
title_short BICEP Array cryostat and mount design
title_full BICEP Array cryostat and mount design
title_fullStr BICEP Array cryostat and mount design
title_full_unstemmed BICEP Array cryostat and mount design
title_sort bicep array cryostat and mount design
publisher arXiv
publishDate 2018
url https://dx.doi.org/10.48550/arxiv.1808.00569
https://arxiv.org/abs/1808.00569
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1808.00569
_version_ 1766201819499855872