The performance of NbN-based phonon-cooled hot electron bolometric (HEB) qu
asioptical mixers is investigated in the 0.7-3.1 THz frequency range. The d
evices are made from a 3.5-4 nm thick NbN film on high resistivity Si and i
ntegrated with a planar spiral antenna on the same substrate. The length of
the bolometer microbridge is 0.1-0.2 mu m; the width is 1-2 mu m. The best
results of the DSB receiver noise temperature measured at 1.5 GHz intermed
iate frequency are: 800 K at 0.7 THz, 1100 K at 1.6 THz, 2000 K at 2.5 THz
and 4200 K at 3.1 THz. The measurements were performed with a far infrared
laser as the local oscillator (LO) source. The estimated LO power requireme
nt is less than 500 nW at the receiver input. First results on spiral anten
na polarization measurements are reported.