2007ApJ...670..206V

The Sloan Digital Sky Survey (SDSS) and photometric/spectroscopic surveys in the GOODS-South field (the Chandra Deep Field-South, CDF-S) are used to construct volume-limited, stellar-mass-selected samples of galaxies at redshifts 0<z<1. The CDF-S sample at 0.6<z<1.0 contains 207 galaxies complete down to M=4x10¹⁰ M_☉(for a ``diet'' Salpeter initial mass function), corresponding to a luminosity limit for red galaxies of M<sub>B</sub>=-20.1. The SDSS sample at 0.020<z<0.045 contains 2003 galaxies down to the same mass limit, which corresponds to M<sub>B</sub>=-19.3 for red galaxies. Morphologies are determined with an automated method, using the Sérsic parameter n and a measure of the residual from the model fits, called ``bumpiness'', to distinguish different morphologies. These classifications are verified with visual classifications. In agreement with previous studies, 65%-70% of the galaxies are located on the red sequence, both at z∼0.03 and at z∼0.8. Similarly, 65%-70% of the galaxies have n>2.5. The fraction of E+S0 galaxies is 43%±3% at z∼0.03 and 48%±7% at z∼0.8; i.e., it has not changed significantly since z∼0.8. When combined with recent results for cluster galaxies in the same redshift range, we find that the morphology-density relation for galaxies more massive than 0.5M^* has remained constant since at least z∼0.8. This implies that galaxies evolve in mass, morphology, and density such that the morphology-density relation does not change. In particular, the decline of star formation activity and the accompanying increase in the stellar mass density of red galaxies since z∼1 must happen without large changes in the early-type galaxy fraction in a given environment.