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Instrumentation for Kinetic Inductance Detector Based Submillimeter Radio Astronomy

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Figure

Figure 1.1: Integrated brightness in cosmic optical, infrared, and microwave background radiation.Reprinted from reference [1].
Figure 1.2:Photographs of the various components of the telescope instrument. (Upper left) Thedetector wafer that serves as the camera of the telescope instrument
Figure 1.4: Scaled version of the antenna, BPF network, and KID layout. (Upper right) A phased-array antenna with a binary summing tree is used to capture the signal
Figure 1.5: Mask design: layout of the major components on the wafer. Plot courtesy of the MUSICgroup.
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