Arid
DOI10.1117/12.926354
The POLARBEAR Experiment
Kermish, Zigmund D.1; Ade, Peter2; Anthony, Aubra3; Arnold, Kam1; Barron, Darcy4; Boettger, David4; Borrill, Julian5,6; Chapman, Scott14; Chinone, Yuji7; Dobbs, Matt A.8; Errard, Josquin9; Fabbian, Giulio9; Flanigan, Daniel1; Fuller, George; Ghribi, Adnan1; Grainger, Will15; Halverson, Nils5; Hasegawa, Masaya7; Hattori, Kaori7; Hazumi, Masashi7; Holzapfel, William L.1; Howard, Jacob1; Hyland, Peter13; Jaffe, Andrew10; Keating, Brian4; Kisner, Theodore5; Lee, Adrian T.1; Le Jeune, Maude9; Linder, Eric11; Lungu, Marius1; Matsuda, Frederick4; Matsumura, Tomotake7; Meng, Xiaofan1; Miller, Nathan J.4; Morii, Hideki7; Moyerman, Stephanie4; Myers, Mike J.1; Nishino, Haruki1; Paar, Hans4; Quealy, Erin1; Reichardt, Christian L.1; Richards, Paul. L.1; Ross, Colin14; Shimizu, Akie7; Shimon, Meir4; Shimmin, Chase1; Sholl, Mike11; Siritanasak, Praween4; Spieler, Helmuth11; Stebor, Nathan4; Steinbach, Bryan1; Stompor, Radek9; Suzuki, Aritoki1; Tomaru, Takayuki7; Tucker, Carole2; Zahn, Oliver11,12
通讯作者Kermish, Zigmund D.
会议名称Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI
会议日期JUL 03-06, 2012
会议地点Amsterdam, NETHERLANDS
英文摘要

We present the design and characterization of the POLARBEAR experiment. POLARBEAR will measure the polarization of the cosmic microwave background (CMB) on angular scales ranging from the experiment's 3.5' beam size to several degrees. The experiment utilizes a unique focal plane of 1,274 antenna-coupled, polarization sensitive TES bolometers cooled to 250 milliKelvin. Employing this focal plane along with stringent control over systematic errors, POLARBEAR has the sensitivity to detect the expected small scale B-mode signal due to gravitational lensing and search for the large scale B-mode signal from inflationary gravitational waves.


POLARBEAR was assembled for an engineering run in the Inyo Mountains of California in 2010 and was deployed in late 2011 to the Atacama Desert in Chile. An overview of the instrument is presented along with characterization results from observations in Chile.


英文关键词Cosmic Microwave Background Inflation Polarization Bolometer
来源出版物MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VI
ISSN0277-786X
出版年2012
卷号8452
EISBN978-0-8194-9153-4
出版者SPIE-INT SOC OPTICAL ENGINEERING
类型Proceedings Paper
语种英语
国家USA;Wales;Japan;Canada;France;England
收录类别CPCI-S
WOS记录号WOS:000312884000039
WOS关键词MICROWAVE BACKGROUND POLARIZATION ; INFLATIONARY UNIVERSE ; FLATNESS ; HORIZON
WOS类目Astronomy & Astrophysics ; Instruments & Instrumentation ; Optics
WOS研究方向Astronomy & Astrophysics ; Instruments & Instrumentation ; Optics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/300881
作者单位1.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA;
2.Cardiff Univ, Sch Phys & Astron, Cardiff, Wales;
3.Univ Colorado, Dept Astrophys & Planetary Sci, Colorado Springs, CO USA;
4.Univ Calif, Dept Phys, San Diego, CA USA;
5.Computat Cosmol Ctr, Lawrence Berkeley Natl Lab, Lawrence, KS USA;
6.Univ Calif, Space Sci Lab, Berkeley, CA USA;
7.High Energy Accelerator Res Org KEK, Tokyo, Japan;
8.McGill Univ, Dept Phys, Montreal, PQ, Canada;
9.Univ Paris 07, APC, Lab Astroparticule & Cosmol, Paris, France;
10.Imperial Coll, Dept Phys, London, England;
11.Lawrence Berkeley Natl Lab, Div Phys, Lawrence, KS USA;
12.Univ Calif, Berkeley Ctr Cosmol Phys BCCP, Berkeley, CA USA;
13.Austin Coll, Dept Phys, Austin, TX USA;
14.Dalhousie Univ, Dept Phys, Halifax, NS, Canada;
15.STFC, Rutherford Appleton Lab, Oxford, England
推荐引用方式
GB/T 7714
Kermish, Zigmund D.,Ade, Peter,Anthony, Aubra,et al. The POLARBEAR Experiment[C]:SPIE-INT SOC OPTICAL ENGINEERING,2012.
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