Ultralow-noise infrared focal plane array status

Details Ultralow-noise infrared focal plane array status Ultralow-noise infrared focal plane array status

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998spie.3436..162k&link_type=abstract

Proc. SPIE Vol. 3436, p. 162-171, Infrared Technology and Applications XXIV, Bjorn F. Andresen; Marija Strojnik Scholl; Eds.

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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.

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