Large area surveys will dominate the forthcoming decades of astronomy and their success requires characterizing thousands of discoveries through additional observations at higher spatial or spectral resolution, and at complementary cadences or periods. Only the full automation of adaptive optics systems will enable high-acuity, high-sensitivity follow-up observations of several tens of thousands of these objects per year, maximizing on-sky time. Automation will also enable rapid response to target-of-opportunity events within minutes, minimizing the time between discovery and characterization. In June 2012, we demonstrated the first fully automated operation of an astronomical adaptive optics system by observing 125 objects in succession with the Robo-AO system. Efficiency has increased ever since, with a typical night comprising 200-250 automated observations at the visible diffraction limit. By observing tens of thousands of targets in the largest-ever adaptive-optics surveys, Robo-AO has demonstrated the ability to address the follow-up needs of current and future large astronomical surveys.
@article{arxiv.1709.07103,
title = {Automated Adaptive Optics},
author = {Christoph Baranec and Reed Riddle and Nicholas M. Law},
journal= {arXiv preprint arXiv:1709.07103},
year = {2021}
}
Comments
Preprint of an article submitted for consideration in The WSPC Handbook of Astronomical Instrumentation http://www.worldscientific.com/worldscibooks/10.1142/9446