The Robo-AO-2 facility for rapid visible/near-infrared AO imaging and the demonstration of hybrid techniques
Christoph Baranec, Mark Chun, Donald Hall, Michael Connelley, Klaus, Hodapp, Daniel Huber, Michael Liu, Eugene Magnier, Karen Meech, Marianne, Takamiya, Richard Griffiths, Reed Riddle, Richard Dekany, Mansi Kasliwal,, Ryan Lau, Nicholas M. Law, Olivier Guyon, Imke de Pater

TL;DR
Robo-AO-2 is a next-generation laser adaptive optics system designed for rapid, high-quality visible and near-infrared imaging, incorporating hybrid techniques to improve faintness limits for exoplanet observations.
Contribution
This paper introduces Robo-AO-2, a new adaptive optics system with hybrid techniques and enhanced capabilities for high-priority astronomical observations.
Findings
Successful development of a reconfigurable guide star sensor
Demonstration of hybrid AO techniques extending faintness limits
Enhanced imaging speed and quality at Maunakea
Abstract
We are building a next-generation laser adaptive optics system, Robo-AO-2, for the UH 2.2-m telescope that will deliver robotic, diffraction-limited observations at visible and near-infrared wavelengths in unprecedented numbers. The superior Maunakea observing site, expanded spectral range and rapid response to high-priority events represent a significant advance over the prototype. Robo-AO-2 will include a new reconfigurable natural guide star sensor for exquisite wavefront correction on bright targets and the demonstration of potentially transformative hybrid AO techniques that promise to extend the faintness limit on current and future exoplanet adaptive optics systems.
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