Michael Bottom,1 Charles-Antoine Claveau,1 Shane Jacobson,1,2 Guillaume Huber,1 Matthew Newland,3 Ian Bakerhttps://orcid.org/0000-0001-6265-9837,4 Keith Barnes,4 Matthew Hicks,4 Angelu Ramos3
1Institute for Astronomy (United States) 2Gemini Observatory (United States) 3Univ. of Hawai'i at Hilo (United States) 4Leonardo UK Ltd. (United Kingdom)
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
We present progress towards developing a science-grade, megapixel format linear-mode avalanche photodiode array for low background shortwave (1 - 2.4 um) infrared astronomy. Our latest results show outstanding performance, with dark current <1e-4 electrons/pixel/second and read noise reducing by 30% per volt of bias, reaching less than 1e-/pixel/frame in correlated double-sampling, and able to average down to ~0.3 e-/pixel/frame when using multiple non-destructive reads. We present some on-sky data as well as comment on prospects for photon counting and photon number resolution.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Michael Bottom, Charles-Antoine Claveau, Shane Jacobson, Guillaume Huber, Matthew Newland, Ian Baker, Keith Barnes, Matthew Hicks, Angelu Ramos, "Progress towards a megapixel linear-mode avalanche photodiode array for ultra-low background shortwave infrared astronomy," Proc. SPIE PC13103, X-Ray, Optical, and Infrared Detectors for Astronomy XI, PC131030D (28 August 2024); https://doi.org/10.1117/12.3020425