Search Results - "Tamazouzt, F."

A 520-620-GHz Schottky Receiver Front-End for Planetary Science and Remote Sensing With 1070 K-1500 K DSB Noise Temperature at Room Temperature by Treuttel, J., Gatilova, L., Maestrini, A., Moro-Melgar, D., Yang, F., Tamazouzt, F., Vacelet, T., Jin, Y., Cavanna, A., Mateos, J., Feret, A., Chaumont, C., Goldstein, C.

“…A state-of-the-art 520-620-GHz receiver front end working at room temperature was designed, built, and measured. The receiver front-end features a…”
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A 330 GHz frequency doubler using European MMIC Schottky process based on e-beam lithography by Treuttel, J., Gatilova, L., Yang, F., Maestrini, A., Jin, Y., Cavanna, A., Vacelet, T., Tamazouzt, F., Krieg, J.-M, Goldstein, C.

“…The Submillimetre-Wave Instrument (SWI) is a passive microwave spectrometer included in the large-class mission in ESA's Cosmic Vision JUpiter ICy moons…”
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