Poster + Paper
29 August 2022 An updated preliminary optical design and performance analysis of the Planetary Systems Imager adaptive optics system
Author Affiliations +
Conference Poster
Abstract
The Planetary Systems Imager (PSI), a proposed instrument suite for the Thirty Meter Telescope (TMT), enables a broad range of extreme-AO, high-contrast observations. PSI is specifically optimized for high contrast exoplanet science from 0.5 to 13 μm and to that end includes a core near-IR AO system that feeds multiple AO+science instrument subsystems. In this paper, we present a preliminary optical design for the full PSI-AO system, feeding the PSI-Red (2—5 μm), PSI-Blue (0.5-–1.8 μm), and PSI-10 (8—13 μm) subsystems. We discuss an initial concept of testing and operations for the system that feeds into the conceptual design. We build on our preliminary end-to-end PSI-Red AO simulation to estimate the raw planet-to-star contrast ratios associated with PSI-Red and extrapolate these results to represent the effects of a PSI-Blue deformable mirror.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rebecca Jensen-Clem, Philip M. Hinz, M. A. M. van Kooten, Michael P. Fitzgerald, Steph Sallum, Benjamin A. Mazin, Mark Chun, Maxwell A. Millar-Blanchaer, Andy Skemer, Ji Wang, R. Deno Stelter, and Olivier Guyon "An updated preliminary optical design and performance analysis of the Planetary Systems Imager adaptive optics system", Proc. SPIE 12185, Adaptive Optics Systems VIII, 1218546 (29 August 2022); https://doi.org/10.1117/12.2630526
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Adaptive optics

Actuators

Wavefronts

Imaging systems

Coronagraphy

Optical design

Wavefront sensors

RELATED CONTENT


Back to Top