Next Talk: May 26
Abstract:   
Studies of galaxies in the early universe (z > 1) have greatly
benefited from recent advances in diffraction-limited techniques on
8-10m telescopes using adaptive optics and integral field spectroscopy. I will present
results from an on-going survey using Keck's latest instrument OSIRIS
and adaptive optics to study the dynamics and chemical abundances of z~1.5
star forming galaxies. I will discuss kinematics and properties of
both merger and disk candidates within our sample, and their significance in the
galaxy formation framework. An unexpected discovery through our study
has been spatially concentrated [NII] and [OIII] emission, and peak line
ratios, like [NII]/H-alpha, that are best explained by the presence of
weak AGN. These are among the weakest known AGN at this epoch, and I will discuss
their potential impact on metallicity studies and explore the high
redshift AGN luminosity function. Lastly, I will discuss the future of AO
instrumentation on extremely large telescopes (30m), and the benefits
these instruments offer for studying galaxy formation and evolution.