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The Primordial Anisotropy Polarization Pathfinder Array (PAPPA): Instrument Overview and Status

机译:原始各向异性极化轨迹阵列(PAPPA):仪器概述和状态

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PAPPA is a balloon-based experiment designed to measure the polarization of the Cosmic Microwave Background using candidate technology for an eventual Einstein Inflation Probe mission. It will survey a 20° x 20° patch of sky with 0.5° angular resolution covering 3 passbands centered at 89, 212 and 302 GHz. Detection will be accomplished via antenna-coupled transition edge sensors (TESs) with SQUID-based readouts. In the eventual flight package, band denning filters and MEMS-based polarization modulators will be incorporated into the superconducting microstrip transmission lines that terminate in resistors that are thermally coupled to the TESs. The MEMS switches will allow on-chip polarization modulation that is faster than significant detector gain variations. The initial configuration will incorporate a simplified focal plane augmented by quasioptical polarization modulation. We describe the overall instrument design and present a summary of the current progress.
机译:Pappa是一个基于气球的实验,旨在使用候选技术来测量宇宙微波背景的极化,以实现最终的爱因斯坦通胀探针使命。它将调查20°x 20°的天空,其覆盖在89,212和302 GHz的3个通带的0.5°角分辨率。通过用基于鱿鱼的读出通过天线耦合的过渡边缘传感器(TES)来完成检测。在最终的飞行包中,频带丹恩滤波器和基于MEMS的偏振调制器将结合到终止于热耦合到苔丝的电阻器中的超导微带传输线中。 MEMS开关将允许片上偏振调制,其比显着的检测器增益变化更快。初始配置将包含由拟光学偏振调制增强的简化焦平面。我们描述了整体仪器设计,并概述了当前进展的摘要。

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