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 investigate the environmental dependence of stellar population properties of galaxies in
the local Universe. Physical quantities related to the stellar content of galaxies are derived …

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 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 …

We use photometric redshifts to analyse the effect of local environment on galaxy colours at
redshifts z≲ 0.63 in the Sloan Digital Sky Survey (SDSS) data release 6 (DR6). We construct …

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 assemble a sample of 3258 low-redshift galaxies from the Sloan Digital Sky Survey Data
Release 6 with complementary photometric observations by the Galaxy Evolution Explorer …