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Antenna-Coupled TES Bolometer Arrays for CMB Polarimetry

机译:用于CMB偏光仪的天线耦合TES阵列阵列

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摘要

We describe the design and performance of polarization selective antenna-coupled TES arrays that will be usedin several upcoming Cosmic Microwave Background (CMB) experiments: SPIDER, BICEP-2/SPUD. The fullylithographic polarimeter arrays utilize planar phased-antennas for collimation (F/4 beam) and microstrip filtersfor band definition (25% bandwidth). These devices demonstrate high optical efficiency, excellent beam shapes,and well-defined spectral bands. The dual-polarization antennas provide well-matched beams and low crosspolarization response, both important for high-fidelity polarization measurements. These devices have so farbeen developed for the 100 GHz and 150 GHz bands, two premier millimeter-wave atmospheric windows forCMB observations. In the near future, the flexible microstrip-coupled architecture can provide photon noise-limited detection for the entire frequency range of the CMBPOL mission. This paper is a summary of theprogress we have made since the 2006 SPIE meeting in Orlando, FL.
机译:我们描述了偏振选择性天线耦合的TES阵列的设计和性能,该阵列将使用几种即将到来的宇宙微波背景(CMB)实验:蜘蛛,二折s-2 / spud。校准偏振仪阵列利用平面相控 - 用于准直(F / 4梁)和微带滤波器的频带定义(25%带宽)。这些器件展示了高光学效率,优异的光束形状和明确定义的光谱带。双偏振天线提供良好匹配的光束和低通配响应,这对于高保真极化测量非常重要。这款器件为100 GHz和150 GHz频段开发了这么福尔邦,两个首屈一指的毫米波大气窗户FORCMB观察。在不久的将来,灵活的微带耦合架构可以为CMBPol任务的整个频率范围提供光子噪声限制检测。本文是自2006年奥兰多的2006年SPIE会议以来,我们制造了Progress的摘要。

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