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dc.contributor.authorHaffert, S.Y.
dc.contributor.authorMales, J.R.
dc.contributor.authorClose, L.M.
dc.contributor.authorVan Gorkom, K.
dc.contributor.authorLong, J.D.
dc.contributor.authorHedglen, A.D.
dc.contributor.authorGuyon, O.
dc.contributor.authorSchatz, L.
dc.contributor.authorKautz, M.
dc.contributor.authorLumbres, J.
dc.contributor.authorRodack, A.
dc.contributor.authorKnight, J.M.
dc.contributor.authorSun, H.
dc.contributor.authorFogarty, K.
dc.date.accessioned2021-08-13T20:56:07Z
dc.date.available2021-08-13T20:56:07Z
dc.date.issued2021
dc.identifier.citationHaffert, S. Y., Males, J. R., Close, L. M., Van Gorkom, K., Long, J. D., Hedglen, A. D., Guyon, O., Schatz, L., Kautz, M., Lumbres, J., Rodack, A., Knight, J. M., Sun, H., & Fogarty, K. (2021). Data-driven subspace predictive control of adaptive optics for high-contrast imaging. Journal of Astronomical Telescopes, Instruments, and Systems, 7(2).
dc.identifier.issn2329-4124
dc.identifier.doi10.1117/1.JATIS.7.2.029001
dc.identifier.urihttp://hdl.handle.net/10150/661198
dc.description.abstractThe search for exoplanets is pushing adaptive optics (AO) systems on ground-based telescopes to their limits. One of the major limitations at small angular separations, exactly where exoplanets are predicted to be, is the servo-lag of the AO systems. The servo-lag error can be reduced with predictive control where the control is based on the future state of the atmospheric disturbance. We propose to use a linear data-driven integral predictive controller based on subspace methods that are updated in real time. The new controller only uses the measured wavefront errors and the changes in the deformable mirror commands, which allows for closed-loop operation without requiring pseudo-open loop reconstruction. This enables operation with non-linear wavefront sensors such as the pyramid wavefront sensor. We show that the proposed controller performs near-optimal control in simulations for both stationary and non-stationary disturbances and that we are able to gain several orders of magnitude in raw contrast. The algorithm has been demonstrated in the lab with MagAO-X, where we gain more than two orders of magnitude in contrast. © 2021 Society of Photo-Optical Instrumentation Engineers (SPIE).
dc.language.isoen
dc.publisherSPIE
dc.rightsCopyright © 2021 SPIE.
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectadaptive optics
dc.subjectcoronagraph
dc.subjectexoplanets
dc.subjecthigh-contrast imaging
dc.subjectspectroscopy
dc.titleData-driven subspace predictive control of adaptive optics for high-contrast imaging
dc.typeArticle
dc.typetext
dc.contributor.departmentUniversity of Arizona, Wyant College of Optical Science
dc.contributor.departmentUniversity of Arizona, Steward Observatory
dc.identifier.journalJournal of Astronomical Telescopes, Instruments, and Systems
dc.description.noteImmediate access
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleJournal of Astronomical Telescopes, Instruments, and Systems
refterms.dateFOA2021-08-13T20:56:07Z


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