Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, 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 …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …

We present the most significant measurement of the cosmic microwave background (CMB)
lensing potential to date (at a level of 40σ), using temperature and polarization data from the …

We investigate the effect of ram-pressure from the intracluster medium on the stripping of H i
gas in galaxies in a massive, relaxed, X-ray bright, galaxy cluster at z= 0.2 from the Blind …

Using the latest cosmological hydrodynamic N-body simulations of groups and clusters, we
study how location in phase-space coordinates at z= 0 can provide information on …

Star-forming galaxies can in principle be transformed into passive systems by a multitude of
processes that quench star formation, such as the halting of gas accretion (starvation) or the …

Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …

It is well known that galaxies falling into clusters can experience gas stripping due to ram
pressure by the intra-cluster medium. The most spectacular examples are galaxies with …

We derive 2D dust attenuation maps at∼ 1 kpc resolution from the UV continuum for 10
galaxies on the z∼ 2 star-forming main sequence (SFMS). Comparison with IR data shows …