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- W2003293757 abstract "A 492 GHz quasioptical superconductor-insulator-superconductor (SIS) heterodyne receiver for submillimeter astronomy has been constructed with a double-sideband noise temperature of 170±25 K, where the system response is an average over a 600 MHz i.f. bandwidth centered at 1.5 GHz. The excellent sensitivity is achieved through use of a planar twin-slot antenna feeding a pair of Nb–Al2O3–Nb junctions linked by an inductance. A main beam of f/15 has been measured. The performance of this receiver is comparable to that of the best 492 GHz waveguide receivers currently in operation." @default.
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- W2003293757 date "1994-06-01" @default.
- W2003293757 modified "2023-09-23" @default.
- W2003293757 title "A 492 GHz quasioptical SIS receiver for submillimeter astronomy" @default.
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- W2003293757 doi "https://doi.org/10.1063/1.1144831" @default.
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