| タイトル | The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz Detector Array of Bolometric Polarimeters |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140017649 |
| 著者（英） | Wollack, Edward; Ali, Aamir; Boone, Fletcher; Bennett, Charles L.; Dunner, Rolando; Halpern, Mark; Stevenson, Thomas; Miller, Nathan; Eimer, Joseph; Colazo, Felipe; Amiri, Mandana; Chan, Manwei; Kogut, Alan J..; Harrington, Kathleen; Crowe, Erik; Cho, Hsiao-Mei; Towner, Deborah; U-Yen, Kongpop; Gothe, Dominik; Denis, Kevin; Moseley, Samuel H.; Chuss, David T.; Appel, John W.; Essinger-Hileman, Thomas; Araujo, Derek |
| 発行日 | 2014-07-23 |
| 言語 | eng |
| 内容記述 | The Cosmology Large Angular Scale Surveyor (CLASS) experiment aims to map the polarization of the Cosmic Microwave Background (CMB) at angular scales larger than a few degrees. Operating from Cerro Toco in the Atacama Desert of Chile, it will observe over 65% of the sky at 38, 93, 148, and 217 GHz. In this paper we discuss the design, construction, and characterization of the CLASS 38 GHz detector focal plane, the first ever Q-band bolometric polarimeter array. |
| NASA分類 | Astrophysics |
| レポートNO | GSFC-E-DAA-TN17264 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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