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Assembly and Integration Process of the First High Density Detector Array for the Atacama Cosmology Telescope

机译:阿塔卡马宇宙望远镜第一个高密度探测器阵列的组装和集成过程

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The Advanced ACTPol (AdvACT) upgrade on the Atacama Cosmology Telescope (ACT) consists of multichroic Transition Edge Sensor (TES) detector arrays to measure the Cosmic Microwave Background (CMB) polarization anisotropies in multiple frequency bands. The first AdvACT detector array, sensitive to both 150 and 230 GHz, is fabricated on a 150 mm diameter wafer and read out with a completely different scheme compared to ACTPol. Approximately 2000 TES bolometers are packed into the wafer leading to both a much denser detector density and readout circuitry. The demonstration of the assembly and integration of the AdvACT arrays is important for the next generation CMB experiments, which will continue to increase the pixel number and density. We present the detailed assembly process of the first AdvACT detector array.
机译:阿塔卡马宇宙望远镜(ACT)上的Advanced ACTPol(AdvACT)升级由多色过渡边缘传感器(TES)检测器阵列组成,可测量多个频带中的宇宙微波背景(CMB)极化各向异性。第一个AdvACT检测器阵列对150 GHz和230 GHz都敏感,被制造在直径为150 mm的晶片上,并且与ACTPol相比,其读出方案完全不同。大约2000个TES测辐射热计被包装到晶片中,导致密度更高的检测器密度和读出电路。 AdvACT阵列的组装和集成演示对于下一代CMB实验至关重要,它将继续增加像素数量和密度。我们介绍了第一个AdvACT检测器阵列的详细组装过程。

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