Presentation + Paper
29 August 2022 Sub-electron noise infrared camera development using Leonardo large format 2Kx2K SWIR LmAPD array
Author Affiliations +
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 (320x256/24μm), was designed by Leonardo UK Ltd specifically for SWIR astronomical applications requiring speed and sensitivity. In the past decade there has been a significant development effort to make larger LmAPD arrays for low-background astronomy and advance adaptive optics.

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 array funded by NASA and a 2K x 2K device funded by ESA for general scientific imaging applications. The 2048x2048 pixel ROIC has a pitch of 15 microns, 4/8/16 outputs and a maximum frame rate of 10 Hz.

The ROIC characterization is scheduled in the third quarter of 2022, while the first arrays will be fabricated by end-2022. The hybridized arrays will be characterized during end-2022. At this time, First Light Imaging will start the development of an autonomous camera integrating this 2Kx2K LmAPD array, based on the unique experience from the C-RED One camera, the only commercial camera integrating the SAPHIRA SWIR LmAPD array. The main features of this camera is presented. The detector will be embedded in a compact high vacuum cryostat cooled with low vibration pulse at 50-80K which does not require external pumping. If necessary, an active vibration damping system can be added for reducing the array vibrations down to 0.01 micron. Sub-electron readout noise is expected to be achieved with high multiplication gain. Custom cold filters and beam aperture cold baffling will be integrated in the camera.

The large format 2Kx2K ROIC for APD array is funded by ESA under a TDE program with the contract number 000130154/20/NL/AR.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Philippe Feautrier, Jean-Luc Gach, Dan Owton, Matthew Hicks, Ian Baker, Keith Barnes, and David Boutolleau "Sub-electron noise infrared camera development using Leonardo large format 2Kx2K SWIR LmAPD array", Proc. SPIE 12191, X-Ray, Optical, and Infrared Detectors for Astronomy X, 121911R (29 August 2022); https://doi.org/10.1117/12.2630858
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Sensors

Readout integrated circuits

Short wave infrared radiation

Avalanche photodetectors

Astronomy

Optical filters

RELATED CONTENT

MCT APD focal plane arrays for astronomy at CEA-LETI
Proceedings of SPIE (August 05 2016)
Large format high SNR SWIR HgCdTe Si FPA with multiple...
Proceedings of SPIE (April 28 2017)
Design study for the WIYN high-resolution infrared camera
Proceedings of SPIE (September 30 2004)
Performance of the WIYN high-resolution infrared camera
Proceedings of SPIE (July 20 2010)
1-5-um infrared camera of the IAC
Proceedings of SPIE (October 20 1993)

Back to Top