Presentation + Paper
1 September 2021 Data-driven subspace predictive control: lab demonstration and future outlook
Author Affiliations +
Abstract
MagAO-X system is a new adaptive optics for the Magellan Clay 6.5m telescope. MagAO-X has been designed to provide extreme adaptive optics (ExAO) performance in the visible. VIS-X is an integral-field spectrograph specifically designed for MagAO-X, and it will cover the optical spectral range (450 – 900 nm) at high-spectral (R=15.000) and high-spatial resolution (7 mas spaxels) over a 0.525 arsecond field of view. VIS-X will be used to observe accreting protoplanets such as PDS70 b & c. End-to-end simulations show that the combination of MagAO-X with VIS-X is 100 times more sensitive to accreting protoplanets than any other instrument to date. VIS-X can resolve the planetary accretion lines, and therefore constrain the accretion process. The instrument is scheduled to have its first light in Fall 2021. We will show the lab measurements to characterize the spectrograph and its post-processing performance.
Conference Presentation
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sebastiaan Y. Haffert, Jared R. Males, Laird Close, Joseph Long, Lauren Schatz, Kyle van Gorkom, Alexander Hedglen, Jennifer Lumbres, Alexander Rodack, Olivier Guyon, Justin Knight, Maggie Kautz, and Logan Pearce "Data-driven subspace predictive control: lab demonstration and future outlook", Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 1182306 (1 September 2021); https://doi.org/10.1117/12.2594875
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KEYWORDS
Adaptive optics

Telescopes

Autoregressive models

Planets

Reconstruction algorithms

Spectrographs

Actuators

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