The Galaxy Luminosity Function to z = 1:  Results from DEEP



		Christopher Willmer
		  Lick Observatory


Local surveys of galaxies show that there is a clear bi-modal
distribution of galaxy colors, while the first measurements of the
galaxy luminosity function at high z showed that the amount of
evolution of the galaxy luminosity-function is strongly color-dependent.
In this talk I will use DEEP survey data consisting of 5000+ galaxies
with spectroscopic redshifts to z = 1.4 to re-examine the evolution of the
luminosity function as a function of galaxy color.