An 800 GHz NbN Phonon-cooled Hot-electron Bolometer Mixer Receiver

Physics – Condensed Matter – Superconductivity

Scientific paper

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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.

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