We present a new model for computing the spectral evolution of stellar populations at ages
between 1× 105 and 2× 1010 yr at a resolution of 3 Å across the whole wavelength range …

We examine the properties of the host galaxies of 22 623 narrow-line active galactic nuclei
(AGN) with 0.02< z< 0.3 selected from a complete sample of 122 808 galaxies from the …

We present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …

We analyze the bivariate distribution, in color versus absolute magnitude (ur vs. M r), of a
low-redshift sample of galaxies from the Sloan Digital Sky Survey (2400 deg 2, 0.004< z< …

We use a complete sample of galaxies drawn from the Sloan Digital Sky Survey to study
how structure, star formation and nuclear activity depend on local density and on stellar …

We use a complete sample of about 140 000 galaxies from the Sloan Digital Sky Survey
(SDSS) to study the size distribution of galaxies and its dependence on their luminosity …

ABSTRACT I have assembled a diverse sample of galaxies from the literature with far-
ultraviolet (FUV), optical, infrared (IR), and radio luminosities to explore the calibration of …

Using photometry and spectroscopy of 183,487 galaxies from the Sloan Digital Sky Survey,
we present bivariate distributions of pairs of seven galaxy properties: four optical colors …

We use a large sample of galaxies from the Two Micron All Sky Survey (2MASS) and the
Sloan Digital Sky Survey (SDSS) to calculate galaxy luminosity and stellar mass functions in …

Abstract GEMS (Galaxy Evolution from Morphologies and SEDs) is a large-area (800 arcmin
2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys …