Paper
1 September 1992 Low-cost 256 x 256 PtSi infrared array for astronomical applications
Albert M. Fowler, James R. Herring
Author Affiliations +
Abstract
The development of a Platinum Silicide (PtSi) array for use in ground-based astronomy has been the goal of a joint effort between the National Optical Astronomy Observatories (NOAO) and the Hughes Technology Center (HTC). This has been accomplished by the introduction of the SWIR PtSi hybrid array for astronomy. The resulting array has an optical cavity tuned to enhance the internal quantum efficiency at 1.7 microns and the use of hybrid technology produces an array with near 100% effective fill factor. Dark currents are much less than 10 electrons sec-1 and the read noise is 55 - 60 e rms. Although the quantum efficiency is not as high as the exotic materials, the high uniformity, stability, and low cost make this an array worth considering for many astronomy applications.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Albert M. Fowler and James R. Herring "Low-cost 256 x 256 PtSi infrared array for astronomical applications", Proc. SPIE 1685, Infrared Detectors and Focal Plane Arrays II, (1 September 1992); https://doi.org/10.1117/12.137817
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KEYWORDS
Astronomy

Staring arrays

Quantum efficiency

Infrared detectors

Infrared radiation

Sensors

Infrared astronomy

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