宇宙学大角尺度巡天仪 (CLASS)：38 GHz 测辐射热计偏振探测器阵列
天体物理仪器与方法
2015-06-22 v1
摘要
宇宙学大角尺度巡天仪 (CLASS) 实验旨在绘制角尺度大于几度的宇宙微波背景 (CMB) 偏振图。该实验运行于智利阿塔卡马沙漠的 Cerro Toco，将在 38、93、148 和 217 GHz 频段观测超过 65% 的天空。本文讨论了 CLASS 38 GHz 探测器焦平面的设计、构建和表征，这是首个 Q 波段测辐射热计偏振阵列。
引用
@article{arxiv.1408.4789,
title = {The Cosmology Large Angular Scale Surveyor (CLASS): 38 GHz detector array of bolometric polarimeters},
author = {John W. Appel and Aamir Ali and Mandana Amiri and Derek Araujo and Charles L. Bennett and Fletcher Boone and Manwei Chan and Hsiao-Mei Cho and David T. Chuss and Felipe Colazo and Erik Crowe and Kevin Denis and Rolando Dunner and Joseph Eimer and Thomas Essinger-Hileman and Dominik Gothe and Mark Halpern and Kathleen Harrington and Gene Hilton and Gary F. Hinshaw and Caroline Huang and Kent Irwin and Glenn Jones and John Karakla and Alan J. Kogut and David Larson and Michele Limon and Lindsay Lowry and Tobias Marriage and Nicholas Mehrle and Amber D. Miller and Nathan Miller and Samuel H. Moseleyb and Giles Novakh and Carl Reintsemad and Karwan Rostemab and Thomas Stevensonb and Deborah Towner and Kongpop U-Yen and Emily Wagner and Duncan Watts and Edward Wollack and Zhilei Xu and Lingzhen Zeng},
journal= {arXiv preprint arXiv:1408.4789},
year = {2015}
}
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