Ai. Harris et al., FANATIC - AN SIS RADIOMETER FOR RADIO ASTRONOMY FROM 660 TO 695 GHZ, International journal of infrared and millimeter waves, 15(9), 1994, pp. 1465-1480
FANATIC is a compact radiometer optimized for radio astronomy from abo
ut 660 to 695 GHz (lambdalambda 455 - 432 mum). We observed a large nu
mber of molecular and atomic spectral lines from galactic and extragal
actic sources during FANATIC's first run on the James Clerk Maxwell Te
lescope in early March 1994. Double sideband receiver temperatures dur
ing observations were about 800 K (25 hnu/k). The heart of the receive
r is a two-junction Nb/AlO(x)/Nb SIS array fed by a sandwiched V-Anten
na. The junction array and antenna are fabricated together at IRAM's G
renoble SIS laboratory. Each junction has a normal resistance of R(n)
approximately 10 OMEGA, an area of approximately 2 mum2, an individual
radial stub circuit to resonate the capacitance, and a lambda/4 trans
former to match to the antenna. The solid-state local oscillator is a
mm-wave Gunn oscillator followed by a doubler and tripler. The LO dipl
exer is a Martin-Puplett interferometer, which insures that there is a
lways abundant LO power for operation and speedy tuning. The receiver
and telescope coupling optics, LO, dewar, and calibration system fit o
n an 0.6 x 0.8 m optical breadboard.