W. Ewing, F. Shepherd, R Capps, E. Dereniak
Optical Engineering, Vol. 22, Issue 3, 223334, (June 1983) https://doi.org/10.1117/12.7973115
TOPICS: Thermography, Infrared imaging, Infrared radiation, Charge-coupled devices, Infrared telescopes, Infrared astronomy, Diodes, Astronomical instrumentation, Optical sensors, Optical instrument design
An infrared staring mode imaging sensor was designed to operate with the NASA Infrared Telescope Facility (IRTF) at Mauna Kea, Hawaii. The sensor has a 0.5 arc sec spatial resolution over a 10 arc sec field and is matched to the f/35 focal ratio of the telescope. The focal plane device is a back-side illuminated Schottky infrared charge-coupled device (IRCCD) mosaic with a photoresponse from 1 to 5upm. Astronomical observations are reported at 2.2 um where the IRCCD quantum efficiency is substantially greater than values normally reported for the 3.4 to 4.2 um thermal imaging band.