Paper
26 October 1998 Ultralow-noise infrared focal plane array status
Lester J. Kozlowski, John T. Montroy, Kadri Vural, William E. Kleinhans
Author Affiliations +
Abstract
Low-noise pixel-based amplification via sub-micron CMOS is enabling advanced focal plane arrays offering ultra-low read noise for infrared astronomy, wave-front sensing, IR spectroscopy, spaceborne sensors and other discriminating uses. Specifically, we report the achievement of less than 30 e- read noise at video frame rates using capacitive transimpedance amplification and less than 1 e- using an enhanced form of gate modulation. We also compare several low- noise IR FPAs at various cutoff wavelengths from 1.1 micrometer to nearly 17 micrometer.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lester J. Kozlowski, John T. Montroy, Kadri Vural, and William E. Kleinhans "Ultralow-noise infrared focal plane array status", Proc. SPIE 3436, Infrared Technology and Applications XXIV, (26 October 1998); https://doi.org/10.1117/12.328012
Lens.org Logo
CITATIONS
Cited by 9 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Capacitance

Sensors

Staring arrays

Video

Charge-coupled devices

Imaging systems

Amplifiers

RELATED CONTENT


Back to Top