The dark and bright sides of massive early-type galaxies
Massive early-type galaxies constitute an ideal test bed to probe our understanding of galaxy formation and evolution. Their high mass, spheroidal morphology...
DESI is a massively multiplexed fiber-fed spectrograph that will make the nextmajor advance in dark energy in the timeframe 2018-2022. On the Mayalltelescope...
If you do any amount of programming, you have certainly found that at some point during its development your code did not work as expected. Perhaps it simply...
The discovery of the CMB B-mode polarization, a smoking-gun of Universe's inflation
On March 17 the team responsible for the BICEP2 experiment, a CMB telescope located in the South Pole, announced the discovery of the primordial B-mode signal...
The distribution of stellar mass in galaxy clusters over cosmic time
Galaxy clusters are the most massive gravitationally collapsed structures in the universe, and they have important cosmological and astrophysical applications...
The dynamical status of galaxy clusters with high X-ray temperature and diffuse radio emissions
Extended, diffuse radio emission (halos and relics) in galaxy clusters is a rare phenomenon. The origin of these radio sources and their connection with cluster...
The epoch of formation of galaxy disks using extragalactic rings
The Time Inference with MUSE in Extragalactic Rings, TIMER, is a project dedicated to study the central regionsof 24 nearby galaxies with the integral field...
Solar Orbiter is the first mission of the ESA Cosmic Vision program and that has recently been approved at implementation level. It is an M class mission with a...
The evolution of galaxies during the first billion years.
Evolution of galaxies is relatively well known up to z ~ 5, but beyond this limit and regarding the few number of galaxies confirmed by spectroscopy, their...