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Millimeter and Submillimeter Detectors for Astronomy II
We describe a new concept for a detector for the submillimeter and far infrared that uses a distributed hotelectron transition edge sensor (TES) to collect the power from a focal-plane-filling slot antenna array. Because superconducting transmission lines are lossy at frequencies greater than about 1 Thz, the sensors must directly tap the antenna, and therefore must match the antenna impedance (∼ 30 ohms). Each pixel contains many TESs that are all wired in parallel as a single distributed TES,doi:10.1117/12.552440 fatcat:7vu5bkfjk5dv7iazccpnf6reui