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DOI | 10.1117/12.926354 |
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 |
ISSN | 0277-786X |
出版年 | 2012 |
卷号 | 8452 |
EISBN | 978-0-8194-9153-4 |
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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