UnISIS: Laser Guide Star and Natural Guide Star Adaptive Optics System

Abstract

is a versatile adaptive optics system mounted on a large optics bench at the coudé focus of the Mount Wilson 2.5-m telescope. It was designed to have both laser guide star (LGS) and natural guide star (NGS) adaptive optics capabilities. The LGS side of the system relies on a pulsed UV laser with raw power of 30 W capable of creating an artificial laser star via Rayleigh scattering 18 km above the telescope. The LGS system can work at temporal response rates as high as 333 Hz-limited by the UV laser pulse rate-and the NGS system can work at rates up to 1.4 kHz. Each side of the system has its own highspeed wavefront sensor that runs separately, but in the LGS mode the NGS wavefront sensor is converted into a natural star tip-tilt sensor. The deformable mirror is conjugate to the telescope's primary mirror and has one of the most densely packed sets of actuators of any adaptive optics system currently in operation. This paper provides details of the UnISIS design and describes key updates we have made to the system. We show NGS AO-corrected images from the sky from the 900 nm z-band through the 2.12 μm K s band. The highest NGS Strehl achieved to date is 0.67 at K s band.

Astronomical adaptive optics: a review

“…The University of Illinois Seeing Improvement System(UnISIS) is a LGS AO system operating at the 2.5m telescope at Mount Wilson Observatory. It is the first astronomical system to employ a Rayleigh LGS at 351nm [35,36]. The system started construction in 1994 and successfully conducted an open loop test in 2002.…”