Presentation + Paper
9 September 2021 The Planetary Systems Imager adaptive optics system: an initial optical design and performance analysis tool for the PSI-Red AO system
Author Affiliations +
Abstract
The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength instrument suite optimized for high contrast science. PSI's broad range of capabilities, spanning imaging, polarimetry, integral field spectroscopy, and high resolution spectroscopy from 0.6–5 μm, with a potential channel at 10 μm, will enable breakthrough science in the areas of exoplanet formation and evolution. Here, we present a preliminary optical design and performance analysis of the 2–5 μm component of the PSI AO system, which must deliver the wavefront quality necessary to support infrared high contrast science cases.
Conference Presentation
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rebecca Jensen-Clem, Philip Hinz, Maaike von Kooten, Michael P. Fitzgerald, Steph Sallum, Benjamin Mazin, Mark Chun, Claire Max, Maxwell Millar-Blanchaer, Olivier Guyon, Andrew Skemer, R. Deno Stelter, and Ji Wang "The Planetary Systems Imager adaptive optics system: an initial optical design and performance analysis tool for the PSI-Red AO system", Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 1182309 (9 September 2021); https://doi.org/10.1117/12.2594005
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KEYWORDS
Adaptive optics

Relays

Wavefront sensors

Mirrors

Wavefronts

Actuators

Coronagraphy

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