MagAO-X Phase II Upgrades: Implementation and First On-Sky Results of a New Post-AO 1000 Actuator Deformable Mirror
Jay K. Kueny, Kyle Van Gorkom, Maggie Kautz, Sebastiaan Haffert, Jared, R. Males, Alex Hedglen, Laird Close, Eden McEwen, Jialin Li, Joseph D. Long,, Warren Foster, Logan Pearce, Avalon McLeod, Jhen Lumbres, Olivier Guyon,, Joshua Liberman

TL;DR
This paper details the implementation and on-sky testing of a new 1000-actuator deformable mirror in MagAO-X, significantly enhancing its adaptive optics capabilities for high-contrast imaging of circumstellar objects.
Contribution
It introduces a high-actuator-count deformable mirror upgrade for MagAO-X, enabling faster correction speeds and improved non-common path aberration correction.
Findings
Successful installation and characterization of the new DM.
On-sky results demonstrate improved wavefront control performance.
Enhanced contrast and Strehl ratio achieved in recent observations.
Abstract
MagAO-X is the extreme coronagraphic adaptive optics (AO) instrument for the 6.5-meter Magellan Clay telescope and is currently undergoing a comprehensive batch of upgrades. One innovation that the instrument features is a deformable mirror (DM) dedicated for non-common path aberration correction (NCPC) within the coronagraph arm. We recently upgraded the 97 actuator NCPC DM with a 1000 actuator Boston Micromachines Kilo-DM which serves to (1) correct non-common path aberrations which hamper performance at small inner-working angles, (2) facilitate focal-plane wavefront control algorithms (e.g., electric field conjugation) and (3) enable 10 kHz correction speeds (up from 2 kHz) to assist post-AO, real-time low-order wavefront control. We present details on the characterization and installation of this new DM on MagAO-X as part of our efforts to improve deep contrast performance for…
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Taxonomy
TopicsOptical Systems and Laser Technology · Adaptive optics and wavefront sensing · Space Satellite Systems and Control
