The Keck Natural Guide Star Adaptive Optics Facility: capabilities and early science

Physics – Optics

Scientific paper

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Scientific paper

The expected breakthrough in astronomical resolution with the implementation of Adaptive Optics (AO) on the new generation of large, 8-10 m diameter telescopes was clearly demonstrated in February, 1999 with the Natural Guide Star AO facility on the Keck II telescope. These first light images had a full-width-at-half-maximum of 0.04 arcsec at H-band and Strehl ratios up to 30 wavelength. Since first-light we have been engaged in a program to characterize and optimize the system on the sky while carrying out a program to verify the scientific capabilities. The facility is now available to our science community. The purpose of this paper is to provide a brief overview of the facility and its performance. Several science papers in this conference, ranging from planets to galaxies, will further demonstrate the dramatic new scientific capabilities of this facility.

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