Physics – Condensed Matter – Superconductivity
Scientific paper
Jun 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999itas....9.3753k&link_type=abstract
IEEE Transactions on Applied Superconductivity, Volume 9, p. 3753-3756
Physics
Condensed Matter
Superconductivity
22
Scientific paper
We describe a heterodyne receiver developed for astronomical applications to operate in the 350 micron atmospheric window. The waveguide receiver employs a superconductive NbN phonon-cooled hot-electron bolometer mixer. The double sideband receiver noise temperature closely follows 1 K per GHz across 780-870 GHz, with the intermediate frequency centered at 1.4 GHz. The conversion loss is about 15 dB. The receiver was installed for operation at the University of Arizona/Max Planck Institute for Radio Astronomy Submillimeter Telescope facility. The instrument was successfully used to conduct test observations of a number of celestial sources in a number of astronomically important spectral lines.
Blundell Ray
Cherednichenko Sergey
Edward Tong C.-Y.
Gershenzon Eugene
Gol'tsman Gregory
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