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11 September 2015 High-contrast imager for complex aperture telescopes (HiCAT): 3. first lab results with wavefront control
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Abstract
HiCAT is a high-contrast imaging testbed designed to provide complete solutions in wavefront sensing, control and starlight suppression with complex aperture telescopes. The pupil geometry of such observatories includes primary mirror segmentation, central obstruction, and spider vanes, which make the direct imaging of habitable worlds very challenging. The testbed alignment was completed in the summer of 2014, exceeding specifications with a total wavefront error of 12nm rms over a 18mm pupil. The installation of two deformable mirrors for wavefront control is to be completed in the winter of 2015. In this communication, we report on the first testbed results using a classical Lyot coronagraph. We also present the coronagraph design for HiCAT geometry, based on our recent development of Apodized Pupil Lyot Coronagraph (APLC) with shaped-pupil type optimizations. These new APLC-type solutions using two-dimensional shaped-pupil apodizer render the system quasi-insensitive to jitter and low-order aberrations, while improving the performance in terms of inner working angle, bandpass and contrast over a classical APLC.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mamadou N'Diaye, Johan Mazoyer, Élodie Choquet, Laurent Pueyo, Marshall D. Perrin, Sylvain Egron, Lucie Leboulleux, Olivier Levecq, Alexis Carlotti, Chris A. Long, Rachel Lajoie, and Rémi Soummer "High-contrast imager for complex aperture telescopes (HiCAT): 3. first lab results with wavefront control", Proc. SPIE 9605, Techniques and Instrumentation for Detection of Exoplanets VII, 96050I (11 September 2015); https://doi.org/10.1117/12.2188497
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