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The new generation CMB B-mode polarization experiment: POLARBEAR

Errard, J. / Ade, P. A. R. / Anthony, A. / Arnold, K. / Aubin, F. / Boettger, D. / Borrill, J. / Cantalupo, C. / Dobbs, M. A. / Flanigan, D. / Ghribi, A. / Halverson, N. / Hazumi, M. / 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, D. / Reichardt, C. / Schanning, I. / Shimizu, A. / Shimmin, C. / Shimon, M. / Spieler, H. / Steinbach, B. / Stompor, R. / Suzuki, A. / Tomaru, T. / Tran, H. T. / Tucker, C. / Quealy, E. / Richards, P. L. / Zahn, O. - 2010
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.

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