The Laboratory for Adaptive Optics enables exploratory research and development of adaptive optics systems for the next generation of high resolution astronomy instrumentation.

The Laboratory is a component of University of California Observatories, with facilities located on the UC Santa Cruz campus. We develop, assemble, and deploy complex adaptive optics instruments for the world's largest telescopes in support of UC Astronomy, including those at the Keck, Gemini, and Lick Observatories. We have a close affiliation with the UC Center for Adaptive Optics where our educational and outreach activities include hosting PhD thesis research, a summer school on adaptive optics, and seminars and workshops in the AO related fields We actively solicit collaboration with industry and partner observatories to pursue goals benefiting the astronomical AO community.

Our current major projects include:

A new Laser Guide Star Adaptive Optics system for the Shane Telescope on Mount Hamilton
Gemini Planet Imager - An "Extreme" Adaptive Optics system for imaging planets around nearby stars - Now at the Gemini South 8-meter telescope in Chile. See the GPI First Light press release. GPI
Keck Next Generation Adaptive Optics - A laser guidestar AO system for the Keck telescope - High Strehl broad spectrum science imaging and spectroscopy over the near-infrared bands 0.7 to 2.2 microns

Read about our laboratory facilities

Through the CfAO, we host a series of workshops on laser guidestars

The LAO was initiated with a generous grant from the Gordon and Betty Moore Foundation.