Deformable mirror interferometric analysis for the direct imagery of exoplanets
Johan Mazoyer, Rapha\"el Galicher, Pierre Baudoz, Patrick, Lanzoni, Fr\'ed\'eric Zamkotsian, G\'erard Rousset

TL;DR
This paper presents an interferometric analysis of a deformable mirror used in high-contrast exoplanet imaging, focusing on surface characterization, actuator behavior, and defect effects to improve adaptive optics performance.
Contribution
It introduces a detailed interferometric method for analyzing deformable mirror surfaces and actuator interactions, enhancing the understanding of mirror defects and behavior in exoplanet imaging systems.
Findings
Precise surface shape characterization of the deformable mirror.
Analysis of individual actuator behavior and cross-talk effects.
Assessment of surface defects and their impact on wavefront correction.
Abstract
Direct imaging of exoplanet systems requires the use of coronagraphs to reach high contrast levels (10^-8 to 10^-11) at small angular separations (0.1"). However, the performance of these devices is drastically limited by aberrations (in phase or in amplitude, introduced either by atmosphere or by the optics). Coronagraphs must therefore be combined with extreme adaptive optic systems, composed of a focal plane wavefront sensor and of a high order deformable mirror. These adaptive optic systems must reach a residual error in the corrected wavefront of less than 0.1 nm (RMS) with a rate of 1 kHz. In addition, the surface defects of the deformable mirror, inherent from the fabrication process, must be limited in order to avoid the introduction of amplitude aberrations. An experimental high contrast bench has been developed at the Paris Observatory (LESIA). This bench includes a Boston…
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