Sub-electron noise infrared camera development using Leonardo large format 2Kx2K SWIR LmAPD array
Philippe Feautrier, Jean-Luc Gach, Dan Owton, Matthew Hicks, Ian, Baker, Keith Barnes, David Boutolleau

TL;DR
This paper discusses the development of a large-format, sub-electron noise SWIR infrared camera using Leonardo's 2Kx2K LmAPD array, advancing low-noise, high-resolution infrared imaging technology.
Contribution
It introduces the design and upcoming fabrication of a 2Kx2K LmAPD array for ultra-low noise SWIR imaging, and details the development of an autonomous camera system utilizing this array.
Findings
Development of a 2048x2048 pixel ROIC with 15-micron pitch.
Scheduled fabrication and characterization of the array in 2022.
Integration of the array into a compact, autonomous camera system.
Abstract
There have been no significant breakthroughs in infrared imagery since the hybridization of III-V or II-VI narrow-bandgap semiconductors on complementary metal-oxide semiconductor (CMOS) read-out integrated circuits (ROICs). The development of third-generation, linear-mode avalanche photodiode arrays (LmAPDs) using mercury cadmium telluride (MCT) has resulted in a significant sensitivity improvement for short-wave infrared (SWIR) imaging. The first dedicated LmAPD device, called SAPHIRA (320x256/24 microns), was designed by Leonardo UK Ltd specifically for SWIR astronomical applications. In the past decade there has been a significant development effort to make larger LmAPD arrays for low-background astronomy. Larger LmAPD formats for ultra-low noise/flux SWIR imaging, currently under development at Leonardo include a 512 x 512 LmAPD array funded by ESO, MPE and NRC Herzberg, a 1k x 1k…
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Taxonomy
TopicsSuperconducting and THz Device Technology · Advanced Semiconductor Detectors and Materials · Calibration and Measurement Techniques
