Paper
8 July 2018 Developing an infrared APD array camera for near-infrared wavefront sensing
Author Affiliations +
Abstract
We will be upgrading the MMT Observatory’s (MMTO) Adaptive Optics (AO) system with a novel Pyramid Wavefront Sensor (PWFS). Our camera will utilize Leonardo’s SAPHIRA, a low-read-noise electron Avalanche Photodiode (eAPD) array. By observing natural guide stars in the near-infrared, we will improve the sky coverage at the MMTO by an order of magnitude. We have developed a compact cryostat that utilizes Sunpower’s CryoTel MT cryocooler to reduce the SAPHIRA’s dark current and thermal background radiation. Our camera’s cooling performance and cryocooler induced vibrations have been quantified and the results are presented here. Upon characterizing the laboratory performance of our camera at various reverse-bias voltages, this instrument will be integrated with MMTO’s adaptive optics system. The successful implementation of this wavefront sensor will pave the way for future applications using this technology in AO systems of extremely large telescopes.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Adam Butko, Suresh Sivanandam, Tim Hardy, Siqi Liu, Shaojie Chen, Jean-Pierre Veran, and Philip M. Hinz "Developing an infrared APD array camera for near-infrared wavefront sensing", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107023N (8 July 2018); https://doi.org/10.1117/12.2314367
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Cited by 1 scholarly publication.
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KEYWORDS
Sensors

Cryocoolers

Cameras

Wavefront sensors

Adaptive optics

Infrared sensors

Wavefronts

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