@Article{Kawamura_etal1999,
author="Kawamura, J. H.
and Tong, C-Y E.
and Blundell, R.
and Cosmo Papa, D.
and Hunter, T. R.
and Gol{\textquoteright}tsman, G.
and Cherednichenko, S.
and Voronov, B.
and Gershenzon, E.",
title="An 800 GHz NbN phonon-cooled hot-electron bolometer mixer receiver",
journal="IEEE Trans. Appl. Supercond.",
year="1999",
volume="9",
number="2",
pages="3753--3756",
optkeywords="NbN HEB mixers",
abstract="We describe a heterodyne receiver developed for astronomical applications to operate in the 350 /spl mu/m atmospheric window. The waveguide receiver employs a superconductive NbN phonon-cooled hot-electron bolometer mixer. The double sideband receiver noise temperature closely follows 1 kGHz/sup -1/ 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.",
optnote="exported from refbase (https://db.rplab.ru/refbase/show.php?record=288), last updated on Tue, 25 May 2021 12:42:38 -0500",
issn="1051-8223",
doi="10.1109/77.783844",
opturl="https://ieeexplore.ieee.org/abstract/document/783844",
opturl="https://doi.org/10.1109/77.783844"
}