@Article{Phillips+Jefferts1973,
author="Phillips, T. G.
and Jefferts, K. B.",
title="A low temperature bolometer heterodyne receiver for Millimeter wave astronomy",
journal="Rev. Sci. Instrum.",
year="1973",
volume="44",
number="8",
pages="1009--1014",
optkeywords="InSb HEB mixer",
abstract="Liquid helium cooled InSb hot electronbolometers are used in a balanced mixer configuration as detectors for an imagelessmicrowave receiver. The system is designed for mounting at the prime focus of the National Radio Astronomy Observatory (NRAO) 11 m antenna at Kitt Peak, Arizona, and is suitable for the study of rotational line spectra of interstellar gas molecules. Currently the operating frequency is in the 90--140 GHz band where the double sideband system noise temperature is 250 K.",
optnote="Recommended by Klapwijk",
optnote="exported from refbase (https://db.rplab.ru/refbase/show.php?record=927), last updated on Tue, 24 Jun 2014 17:17:23 -0500",
doi="10.1063/1.1686288",
opturl="https://doi.org/10.1063/1.1686288"
}