Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

I start by providing an updated summary of the penalized pixel-fitting (ppxf) method that is
used to extract the stellar and gas kinematics, as well as the stellar population of galaxies …

We use cosmological simulations from the FIRE (Feedback In Realistic Environments)
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …

Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics …

Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …

There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

We present the stellar population content of early-type galaxies from the ATLAS3D survey.
Using spectra integrated within apertures covering up to one effective radius, we apply two …

Using the IllustrisTNG simulations, we investigate the connection between galaxy
morphology and star formation in central galaxies with stellar masses in the range 109 …

The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …