Galaxy evolution is one of the key questions in current astronomy.
Observations of strong and recent galaxy evolution conflict with
previous ideas of orderly and early evolution of galaxies.
The purpose of our survey is to obtain an accurate description of the
distribution of magnitude, structural parameters, color, and spectral
type for a large number of field galaxies. Of these galaxies we will
measure star formation rate and star formation history and calculate
detection rates at increasing redshift.
These data will be used as an aid in understanding the spectra of
galaxies at higher redshift, and in measuring the changes in star
formation rates over time.