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BICEP2/SPUD: Searching for inflation with degree scale polarimetry from the South Pole

机译:BICEP2 / SPUD:从南极通过度数极化法搜索通货膨胀

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BICEP2/SPUD is the new powerful upgrade of the existing BICEP1 experiment, a bolometric receiver to study the polarization of the cosmic microwave background radiation, which has been in operation at the South Pole since January 2006. BICEP2 will provide an improvement up to 10 times mapping speed at 150 GHz compared to BICEP1, using the same BICEP telescope mount. SPUD, a series of compact, mechanically-cooled receivers deployed on the DASI mount at the Pole, will provide similar mapping speed in to BICEP2 in three bands, 100, 150, and 220 GHz. The new system will use large TES focal plane arrays to provide unprecedented sensitivity and excellent control of foreground contamination.
机译:BICEP2 / SPUD是现有BICEP1实验的新功能强大升级,BICEP1实验是用于研究宇宙微波背景辐射极化的辐射热接收器,该辐射自2006年1月起在南极投入使用。BICEP2将提供多达10倍的改进使用相同的BICEP望远镜安装座,与BICEP1相比在150 GHz处的最大贴图速度。 SPUD是一系列紧凑,机械冷却的接收器,部署在波兰人的DASI支架上,将在100 GHz,150 GHz和220 GHz三个频段提供与BICEP2相似的映射速度。新系统将使用大型TES焦平面阵列,以提供前所未有的灵敏度和对前景污染的出色控制。

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