Despite the success of the standard LambdaCDM model, it is argued that some modifications may well be motivated on theoretical and observational grounds. The talk will discuss how to…
We have great certainty on how gravity works around our Solar System, but on large scales we still have a considerable lack of understanding about the constituents of our universe. Furthermore…
Today’s massive elliptical galaxies are primarily red-and-dead, dispersion supported ellipticals. The physical process(es) driving the shutdown or “quenching” of star formation in these…
CII is one of the brightest emission lines from star-forming galaxies and is an excellent tracer for star formation. Recent work measured the CII emission line amplitude for redshifts 2<z<3.2…
