Research in Adaptive Optics
Adaptive optics (AO) compensate for the variability of images due to irregularities in the medium through which the light passes. In astronomy, adaptive optics are used to correct for the distortion that is inevitably introduced when objects are viewed through the Earth's turbulent atmosphere, i.e. removing the twinkling of starlight. Without adaptive optics, images taken at ground-based telescopes are typically smeared by half an arcsecond or more, reducing both the resolution of the images and the sensitivity of the telescope since the light is spread over a larger area. One way to improve images is to move above the atmosphere, as the Hubble Space Telescope (HST) has done. But bigger telescopes can be built on Earth far less expensively than HST. Adaptive optics promises resolution four or five times better than HST on existing telescopes like Keck, and potentially far better on the next generation of even larger telescopes.
The Center for Adaptive Optics (CFAO) is a National Science Foundation
Science and Technology Center headquartered on the UCSC campus in a
new building adjacent to the astronomy department. With nearly a dozen
member universities and over a dozen affiliated labs, institutes, and
industrial associates, the CfAO's themes are AO for extremely large
telescopes, extreme AO for ultra-high contrast observations to detect
extra-solar planets, instrumentation for AO in clinical and research
applications in vision science, and education at all levels from the
public to the research community. UCSC faculty associated with CfAO
include the Director, Claire Max, as well as Sandy
Faber, Raja GuhaThakurta, David
Koo, and Jerry Nelson. Many graduate students
and postdocs are also center members.
A complementary Laboratory for Adaptive Optics was recently established at UCSC through a generous gift of the Gordon and Betty Moore Foundation -- the first comprehensive university laboratory dedicated to adaptive optics in the United States. The Laboratory, directed by Dr. Donald Gavel, serves as a test facility for ideas developed at CfAO, allowing researchers to develop and test prototypes of AO equipment in laboratory settings. The Lab is located on the first floor of Thimann Labs, near the CfAO building.
- Faculty
- Rebecca Bernstein
- Michael Bolte
- Jean Brodie
- Harland Epps
- Sandra Faber
- Jonathan Fortney
- Raja Guha Thakurta
- Garth Illingworth
- David Koo
- Mark Krumholz
- Gregory Laughlin
- Douglas Lin
- Piero Madau
- Claire Max
- Joseph Miller
- Jerry Nelson
- Xavier Prochaska
- Enrico Ramirez-Ruiz
- Constance Rockosi
- Graeme Smith
- Stephen Thorsett
- Steven Vogt
- Stan Woosley
- Research Centers
- CfAO
- CODEP
- COSV
- LAO
- PISGM
- PLANETS
- TASC
- SCIPP
- Research Groups
- AEGIS
- CATS
- CCPI
- DEEP2
- First Galaxies
- N2K
- SAGES
- SciDAC
- Splash