We present our latest results based on the Spitzer Cosmological Surveys about the characterization of the mass assembly of galaxies in the last 12 Gyr. We have...

We have developed COSMOPACK, a set of tools that transform images of real galaxies to depict their appearance at a given redshift as observed with a given...

There are two principal problems in explaining, in terms of the emission from OB stars, the ionisation of the gas which emits the diffuse H-alpha in spiral...

Star formation is a vital phenomenon across all fields of astronomy, shaping our universe in all its vastness, from the small scale of exoplanets to the large...

We have studied the quantitative morphology and structural parameters of the bright galaxy population in the Nordic Optical Telescope (NOT) sample, which...

We have developed morphological analysis software for studying galaxies from low to high redshifts. This code is designed to extract quantitative information...

First results of a photometric study of the richness=2 Abell Cluster 2443 at z=0.103 are presented. We have developed a new algorithm to perform a detailed...

We present the results from the quantitative spectroscopic analysis of ~280 likely single O stars targeted by the IACOB and OWN surveys. This implies the...

Massive stars are luminous beacons that help us to extract information about the star formation history and the chemodynamical evolution of galaxies in the...