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Antenna-coupled transition-edge hot-electron microbolometers
2004
Millimeter and Submillimeter Detectors for Astronomy II
We are developing a new type of detector for observational cosmology and astrophysical research. Incoming radiation from the sky is coupled to a superconducting microstrip transmission line that terminates in a thin film absorber. At sub-Kelvin temperature, the thermal isolation between the electrons and the lattice makes it possible for the electrons in the small absorber (100's of µm 3 ) and superconducting bilayer (Transition Edge Sensor) to heat up by the radiation absorbed by the electrons
doi:10.1117/12.552836
fatcat:fbo5wc37l5fvfmrsstganpmp64