Walker S, Sierra C E, Austermann J E, Beall J A, Becker D T, Dober B J, Duff S M, Hilton G C, Hubmayr J, Van Lanen J L, McMahon J J, Simon S M, Ullom J N, Vissers M R
University of Colorado Boulder, Boulder, CO, USA.
National Institute of Standards and Technology, Boulder, CO, USA.
J Low Temp Phys. 2020;199(3-4). doi: 10.1007/s10909-019-02316-1.
We describe the design and measurement of feedhorn-coupled, transition-edge sensor (TES) polarimeters with two passbands centered at 220 GHz and 280 GHz, intended for observations of the cosmic microwave background. Each pixel couples polarized light in two linear polarizations by use of a planar orthomode transducer and senses power via four TES bolometers, one for each band in each linear polarization. Previous designs of this detector architecture incorporated passbands from 27 to 220 GHz; we now demonstrate this technology at frequencies up to 315 GHz. Observational passbands are defined with an on-chip diplexer, and Fourier-transform-spectrometer measurements are in excellent agreement with simulations. We find coupling from feedhorn to TES bolometer using a cryogenic, temperature-controlled thermal source. We determine the optical efficiency of our device is = 77% ± 6% (75% ± 5%) for 220 (280) GHz, relative to the designed passband shapes. Lastly, we compare two power-termination schemes commonly used in wide-bandwidth millimeter-wave polarimeters and find equal performance in terms of optical efficiency and passband shape.
我们描述了用于宇宙微波背景观测的、具有两个分别以220吉赫兹和280吉赫兹为中心的通带的馈源喇叭耦合过渡边传感器(TES)偏振计的设计与测量。每个像素通过使用平面正交模变换器耦合两种线性偏振的偏振光,并通过四个TES测辐射热计感测功率,每个线性偏振的每个波段各有一个测辐射热计。这种探测器架构的先前设计包含27至220吉赫兹的通带;我们现在展示了这种技术在高达315吉赫兹频率下的情况。观测通带由片上双工器定义,傅里叶变换光谱仪测量结果与模拟结果高度吻合。我们使用低温、温度可控的热光源来确定从馈源喇叭到TES测辐射热计的耦合。相对于设计的通带形状,我们确定我们装置在220(280)吉赫兹时的光学效率为77%±6%(75%±5%)。最后,我们比较了宽带毫米波偏振计中常用的两种功率终端方案,发现在光学效率和通带形状方面性能相当。