In recent years, responding to the need of the astronomical community,
superconductor-insulator-superconductor (SIS) mixers have been develo
ped to operate at THz frequencies. Best results are obtained by using
niobium-based tunnel junctions with well-matched low-loss normal metal
striplines, which are found to be less lossy than niobium striplines
operated above the gap frequency of niobium (700 GHz). Niobium nitride
tunnel junctions with a magnesium oxide tunnel barrier, although havi
ng reasonable-quality current-voltage characteristics, have been found
to be unsuitable owing to excess shot noise resulting from pinholes i
n the barrier.