2012-10-30
K. Arnold (1), P.A.R. Ade (2), A.E. Anthony (3), D. Barron (4)D. Boettger (4), J. Borrill (5,6), S. Chapman (7)Y. Chinone (11), M.A. Dobbs (8), J. Errard (10), G. Fabbian (10), D. Flanigan (1), G. Fuller (4), A. Ghribi (1), W. Grainger (13), N. Halverson (3), M. Hasegawa (11), K. Hattori (11)M. Hazumi (11), W.L. Holzapfel (1), J. Howard (1), P. Hyland (9), A. Jaffe (12), B. Keating (4), Z. Kermish (1), T. Kisner (5), M. Le Jeune (10), A.T. Lee (1,12), E. Linder (13), M. Lungu (1), F. Matsuda (4), T. Matsumura (11), N.J. Miller (4), X. Meng (1), H. Morii (11), S. Moyerman (4), M.J. Myers (1), H. Nishino (1), H. Paar (4), E. Quealy (1), C. Reichardt (1), P.L. Richards (1), C. Ross (7), A. Shimizu (11)C. Shimmin (1), M. Shimon (4), M. Sholl (12), P. Siritanasak (4), H. Spieler (12), N. Stebor (4), et al. (6 additional authors not shown)
Abstract
The Polarbear Cosmic Microwave Background (CMB) polarization experiment is currently observing from the Atacama Desert in Northern Chile. It will characterize the expected B-mode polarization due to gravitational lensing of the CMB, and search for the possible B-mode signature of inflationary gravitational waves. Its 250 mK focal plane detector array consists of 1,274 polarization-sensitive antenna-coupled bolometers, each with an associated lithographed band-defining filter. Each detector’s planar antenna structure is coupled to the telescope’s optical system through a contacting dielectric lenslet, an architecture unique in current CMB experiments. We present the initial characterization of this focal plane.
Abstract (translated by Google)
URL
https://arxiv.org/abs/1210.7877
PDF
https://arxiv.org/pdf/1210.7877