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dmkelly42
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Demonstrate contrast on existing instrument MagAO-X
Demonstrate contrast on existing instrument MagAO-X (Mitigation for R-01)
Oct 4, 2022
To meet contrast goals, we need to perform high-quality wavefront sensing and control in the coronagraph loop. LOWFS and CLOWFS methods have been demonstrated and are used routinely. The next big development we need is the implementation of EFC, which was demonstrated on-sky during a MagAO-X run in March 2024. It needs to be improved upon to achieve target contrast goals.
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