Translator Disclaimer
13 September 2005 A new large-well 1024×1024 Si:As detector for the mid-infrared
Author Affiliations +
We present a description of a new 1024×1024 Si:As array designed for ground-based use from 5 - 28 microns. With a maximum well depth of 5e6 electrons, this device brings large-format array technology to bear on ground-based mid-infrared programs, allowing entry to the megapixel realm previously only accessible to the near IR. The multiplexer design features switchable gain, a 256×256 windowing mode for extremely bright sources, and it is two-edge buttable. The device is currently in its final design phase at DRS in Cypress, CA. We anticipate completion of the foundry run in October 2005. This new array will enable wide field, high angular resolution ground-based follow up of targets found by space-based missions such as the Spitzer Space Telescope and the Widefield Infrared Survey Explorer (WISE).
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. K. Mainzer, John Hong, M. G. Stapelbroek, Henry Hogue, Dale Molyneux, Michael E. Ressler, Ernie Atkins, John Reekstin, Mike Werner, and Erick Young "A new large-well 1024×1024 Si:As detector for the mid-infrared", Proc. SPIE 5881, Infrared and Photoelectronic Imagers and Detector Devices, 58810Y (13 September 2005);


Flight performance of the Far-Infrared Line Mapper (FILM)
Proceedings of SPIE (October 21 1996)
Imaging telescope-spectrometer for infrared sky surveys
Proceedings of SPIE (June 12 1995)
The Long Wavelength Spectrometer (LWS) for ISO
Proceedings of SPIE (May 01 1986)
OMEGA IR spectral imager for Mars 96 mission
Proceedings of SPIE (December 15 1995)
Geostationary wedge-filter imager-sounder
Proceedings of SPIE (February 08 2001)

Back to Top