The evidence for the existence of dark energy is conclusive, but its nature remains one of the most puzzling mysteries in all of physics. Astronomical surveys...
From the blue cloud to the red sequence (and over the green valley): investigating the evolution of galaxies over cosmological timescales
In the local universe, galaxies fall into one of two populations: a star-forming blue cloud and a red sequence lacking star formation. At redshift z ~ 1.5...
Galactic archeology of thick discs: excavating ESO 533-4 with VIMOS and ESO 243-49 with MUSE
The disc of galaxies is made of the superposition of a thin and a thick disc. Thick discs are seen in edge-on galaxies as excesses of light a few thin disc...
Galactic Dynamics to Explain Outer Disc Features in Spiral Galaxies
Milky Way and most spiral galaxies present some features in the outer part of its disk such as S-warping or U-warping, flaring, lopsidedness, truncation/non...
I will talk about how resolved stellar populations in the nearby Local Group dwarf galaxies have been used to study the detailed chemical, kinematic and star...
GALAPAGOS in C - computational study of galaxy morphologies
Modern imaging surveys provide a fundamental tool in order to study the morphologicalproperties of galaxy populations in the nearby and the distant Universe. In...
Galaxies and quasars in the early Universe: recent results and future prospects from sub-millimeter observations
In recent years, major changes were done at the IRAM Plateau de Bure interferometer and 30-meter telescope, in particular in the areas of receivers and back...
It has been thirty years since the seminal work of Alan Dressler on the density-morphology relation, which established environment as a driving mechanism for...
Galaxy environments at low- and high-z & Constraining the dust content of tadpoles
One of the important questions in extragalactic astronomy concerns the debate between nature and nurture scenarios. Are the observed galaxy local properties the...