The new generation CMB B-mode polarization experiment: POLARBEAR

Errard, J., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Anthony, A., Arnold, K., Aubin, F., Boettger, D., Borrill, J., Cantalupo, C., Dobbs, M. A., Flanigan, D., Ghribi, A., Halverson, N., Holzapfel, W. L., Howard, J., Hyland, P., Jaffe, A., Keating, B., Kisner, T., Kermish, Z., Lee, A. T., Linder, E., Lungu, M., Matsumura, T., Miller, N., Meng, X., Myers, M., Nishino, H., O'Brient, R., O'Dea, R., Reichardt, C., Schanning, I., Shimizu, A., Shimmin, C., Shimon, M., Spieler, H., Steinbach, B., Stompor, R., Suzuki, A., Tomaru, T., Tran, H. T., Tucker, Carole ORCID: https://orcid.org/0000-0002-1851-3918, Quealy, E., Richards, P. L. and Zahn, O. 2010. The new generation CMB B-mode polarization experiment: POLARBEAR. Presented at: 2010 Rencontres de Moriond, La Thuile, Italy, 6-20 March 2010. Proceedings of Rencontres de Moriond

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Abstract

We describe the Cosmic Microwave Background (CMB) polarization experiment called Polarbear. This experiment will use the dedicated Huan Tran Telescope equipped with a powerful 1,200-bolometer array receiver to map the CMB polarization with unprecedented accuracy. We summarize the experiment, its goals, and current status.

Item Type:	Conference or Workshop Item (Other)
Date Type:	Completion
Status:	Unpublished
Schools:	Schools > Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Last Modified:	21 Oct 2022 09:08
URI:	https://orca.cardiff.ac.uk/id/eprint/35431

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