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arXiv 1408.4789astro-ph.IM
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宇宙学大角尺度探测器（CLASS）：38 GHz测辐射热偏振计探测器阵列

The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters

John W. Appel, Aamir Ali, Mandana Amiri, Derek Araujo, Charles L. Bennett, Fletcher Boone, Manwei Chan, Hsiao-Mei Cho, David T. Chuss, Felipe Colazo, Erik Crowe… 展开作者

John W. Appel, Aamir Ali, Mandana Amiri, Derek Araujo, Charles L. Bennett, Fletcher Boone, Manwei Chan, Hsiao-Mei Cho, David T. Chuss, Felipe Colazo, Erik Crowe, Kevin Denis, Rolando Dunner, Joseph Eimer, Thomas Essinger-Hileman, Dominik Gothe, Mark Halpern, Kathleen Harrington, Gene Hilton, Gary F. Hinshaw, Caroline Huang, Kent Irwin, Glenn Jones, John Karakla, Alan J. Kogut, David Larson, Michele Limon, Lindsay Lowry, Tobias Marriage, Nicholas Mehrle, Amber D. Miller, Nathan Miller, Samuel H. Moseleyb, Giles Novakh, Carl Reintsemad, Karwan Rostemab, Thomas Stevensonb, Deborah Towner, Kongpop U-Yen, Emily Wagner, Duncan Watts, Edward Wollack, Zhilei Xu, Lingzhen Zeng

备注：
15 pages, 4 figures. Presented at SPIE Astronomical Telescopes and Instrumentation 2014: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. To be published in Proceedings of SPIE Volume 9153
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摘要：

宇宙学大角度尺度探测器（CLASS）实验旨在绘制大于几度的角度尺度上的宇宙微波背景（CMB）偏振。它将在智利阿塔卡马沙漠的Cerro Toco工作，在38，93，148和217 GHz的频率下观测超过65%的天空。在本文中，我们讨论的设计，施工和表征的类38 GHz探测器焦平面，有史以来第一个Q波段测辐射热偏振计阵列。

英文摘要：

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.

机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。

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