Status and performance of the THD2 bench in multi-deformable mirror configuration
Pierre Baudoz, Raphael Galicher, Fabien Patru, Olivier Dupuis, Simone, Thijs

TL;DR
The paper presents the design, capabilities, and recent performance evaluation of the THD2 high contrast imaging bench, which is used to test coronagraphs and wavefront control techniques for exoplanet imaging.
Contribution
It introduces the upgraded THD2 bench with multi-deformable mirror configuration and details its application in comparing coronagraph performance.
Findings
Chromatic behavior of various coronagraphs characterized
THD2 bench successfully simulates space telescope beam conditions
Performance comparison informs future exoplanet imaging instrument design
Abstract
The architecture of exoplanetary systems is relatively well known inward to 1 AU thanks to indirect techniques, which have allowed characterization of thousands of exoplanet orbits, masses and sometimes radii. The next step is the characterization of exoplanet atmospheres at long period, which requires direct imaging capability. While the characterization of a handful of young giant planets is feasible with dedicated instruments like SPHERE/VLT, GPI/Gemini, SCExAO/Subaru and soon with the coronagraphic capabilities aboard JWST, the spectroscopic study of mature giant planets and lower mass planets (Neptune-like, Super Earths) requires the achievement of better coronagraphic performance. While space-based coronagraph on WFIRST-AFTA might start this study at low spectroscopic resolution, dedicated projects on large space telescope and on the ELT will be required for a more complete…
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