Galactic Chemical Abundances at Z > 3 I: First Results from the Echellette Spectrograph and Imager

We present the first results from an ongoing survey to discover and measure the metallicity of z > 3 damped Lyα systems with the Echellette Spectrograph and Imager (ESI) on the Keck II telescope. Our motivation arises from a recent study on the damped Lyα systems suggesting only mild evolution in the cosmic metallicity from z ∼ 2 to 4. The Echellette Spectrograph and Imager, which provides two complementary spectroscopic modes, is the ideal instrument for a z > 3 damped Lyα survey. We describe our observing strategy and report on the discovery and analysis of 5 new z > 3 damped Lyα systems acquired in a single night of observing. These observations further support the principal conclusions of the previous study: (1) the cosmic metallicity in neutral gas inferred from the damped Lyα systems does not evolve significantly from z ∼ 2 to 4; (2) the unweighted metallicity exhibits a statistically significant decrease with increasing redshift; and (3) not a single damped Lyα system has a metallicity below [Fe/H] = −3. We discuss the implications of these results and comment on recent theoretical studies which attempt to explain the observations. Subject headings: galaxies: abundances — galaxies: chemical evolution — quasars : absorption lines