A metrological characterization of the SPEED test-bed PIAACMC components
K. Barjot, P. Martinez, M. Beaulieu, C. Gouvret, A. Marcotto, O., Guyon, M. Belhadi, A. Caillat, T. Behaghel, J.M. Le Duigou, K. Dohlen, A., Vigan

TL;DR
This paper presents a detailed metrological characterization of the PIAACMC components for the SPEED test-bed, aiming to enhance high-contrast exoplanet imaging capabilities on future extremely large telescopes.
Contribution
It provides the first comprehensive optical quality assessment of the PIAACMC components using interferential microscopy, informing their integration into the SPEED setup.
Findings
High optical quality of manufacturing components
Metrological data supports precise implementation
Insights for future PIAACMC component improvements
Abstract
The segmented pupil experiment for exoplanet detection (SPEED) facility aims to improve knowledge and insight into various areas required for gearing up high-contrast imaging instruments adapted to the unprecedented high angular resolution and complexity of the forthcoming extremely large telescopes (ELTs). SPEED combines an ELT simulator, cophasing optics, wavefront control and shaping with a multi-deformable mirror (DM) system, and optimized small inner-working angle (IWA) coronagraphy. The fundamental objective of the SPEED setup is to demonstrate deep contrast into a dark hole optimized for small field of view and very small IWA, adapted to the hunt of exoplanets in the habitable zone around late-type stars. SPEED is designed to implement an optimized small IWA coronagraph: the phase-induced amplitude apodization complex mask coronagraph (PIAACMC). The PIAACMC consists in a…
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