email: david at ucolick.org
phone: 831-459-3809
My research interest is centered on using moderate to
high-resolution spectroscopy to perform abundance analysis of very
metal-poor field stars. I currently am working on a sample of
high-resolution spectra from HIRES on Keck with -2<[Fe/H]<-4, from
which I have measured from CNO and up through the neutron-capture
elements. I am also working on a program using the Lick
high-precision planet finding setup to monitor a sample of metal-poor
stars in an attempt to constrain their companion fraction, and studies
of M5 and M92 to look for signs of abundance variations and
evolution. In general I'm interested in using stellar spectroscopy as
a tool to constrain theories of Galaxy formation, star formation, and
supernovae models.