We describe the fabrication and characterization of superconducting transit
ion-edge bolometers for astrophysical applications at far-infrared and mm w
avelengths. The sensor is voltage biased and the current is measured with a
superconducting quantum interference ammeter. Strong negative electrotherm
al feedback keeps the sensor temperature nearly constant, reduces the respo
nse time significantly, and improves linearity. It also makes the responsiv
ity relatively insensitive to changes in optical background loading and ref
rigerator temperature. The bolometers are made using standard microlithogra
phic techniques suitable for fabrication of large scale arrays. Detailed me
asurements of optical response are presented for a range of bias conditions
and are compared with theory. Measured noise spectra are shown and a model
for the noise is presented. (C) 1999 American Institute of Physics. [S0003
-6951(99)04206-0].