High-contrast imager for Complex Aperture Telescopes (HiCAT): 3. first lab results with wavefront control
arXiv:1911.03734 · doi:10.1117/12.2188497
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.
12 pages, 10 figures, Proceedings of the SPIE, Volume 9605, id. 96050I 12 pp. (2015)
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Cited by in corpus (5)
- Active correction of aperture discontinuities - optimized stroke minimization II: optimization for future missions
- Active correction of aperture discontinuities - optimized stroke minimization I: a new adaptive interaction matrix algorithm
- High-contrast imager for complex aperture telescopes (HiCAT): 5. first results with segmented-aperture coronagraph and wavefront control
- Capabilities of ACAD-OSM, an active method for the correction of aperture discontinuities
- Correcting for the effects of pupil discontinuities with the ACAD method