Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …

One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …

Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …

There is growing interest in digital PCR (dPCR) because technological progress makes it a
practical and increasingly affordable technology. dPCR allows the precise quantification of …

We explore the simple inter-relationships between mass, star formation rate, and
environment in the SDSS, zCOSMOS, and other deep surveys. We take a purely empirical …

Satellite galaxies in groups and clusters are more likely to have low star formation rates
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …

We measure the luminosity and color dependence of galaxy clustering in the largest-ever
galaxy redshift survey, the main galaxy sample of the Sloan Digital Sky Survey Seventh Data …

We present an end-to-end, two-phase model for the origin of globular clusters (GCs). In the
model, populations of stellar clusters form in the high-pressure discs of high-redshift (z> 2) …