We develop a new method to constrain the star formation histories, dust attenuation and
stellar masses of galaxies. It is based on two stellar absorption-line indices, the 4000-Å …

We present the results of a moped analysis of∼ 3× 105 galaxy spectra from the Sloan
Digital Sky Survey Data Release 3 (SDSS DR3), with a number of improvements in data …

Using the moped algorithm, we determine non-parametrically the stellar mass function of 96
545 galaxies from the Sloan Digital Sky Survey Data Release One. By using the …

We revisit the bimodal distribution of the galaxy population commonly seen in the local
universe. Here, we address the bimodality observed in galaxy properties in terms of spectral …

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 …

We study the relations between stellar mass, star formation history, size and internal
structure for a complete sample of 122 808 galaxies drawn from the Sloan Digital Sky …

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 …

Using a large galaxy group catalogue constructed from the Sloan Digital Sky Survey Data
Release 2, we investigate the correlation between various galaxy properties and halo mass …

The study of stellar populations in galaxies is entering a new era with the availability of large
and high-quality data bases of both observed galactic spectra and state-of-the-art …

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 …