Office: Kerr 435
The most ambitious project is a major new redshift survey of 50,000 extremely faint galaxies using the Keck Telescope, complemented with sharp images from HST. Called DEEP (Deep Extragalactic Evolutionary Probe), this project starting in year 2000 aims to tackle many fundamental questions in the evolution of distant galaxies, the development of clustering in the universe, and the curvature of space, via several cosmological tests. The survey is distinguished by its attempt to measure the masses of distant galaxies as well as their light. This is a collaborative project with astronomers from several institutions and will include construction of a new powerful spectrograph for Keck.
Another major research program involves participation in a new NSF Science and Technology Center for Adaptive Optics awarded to UC Santa Cruz in summer of 1999 (only five awarded in the nation and the only one in the physical sciences). Adaptive optics is a technique designed to provide diffraction limited images for ground-based telescopes by correcting for the blur of the atmosphere. In principle, such a system, already working on Keck, will provide image quality sharper than that from the HST. This project is also a team effort and is also aimed towards studying the morphologies and masses of distant galaxies.
Koo not only works with one or more graduate students but also with 3-5 postdocs at Santa Cruz. Recent work with graduate students includes exploring galaxy star formation histories from multicolor photometry; tracking the evolution of distant clusters of galaxies; and studying the sizes and shapes of distant galaxies using the HST.
For more information about research, publications and courses taught, please visit David Koo’s website.