Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …

We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS
OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD - IOPscience …

Using cosmological simulations, we address the properties of high-redshift star-forming
galaxies (SFGs) across their main sequence (MS) in the plane of star formation rate (SFR) …

Using cosmological simulations, we address the interplay between structure and star
formation in high-redshift galaxies via the evolution of surface density profiles. Our sample …

We present new measurements of the cosmic cold molecular gas evolution out to redshift 6
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …

We use the results from the ALMA large program ASPECS, the spectroscopic survey in the
Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the …

Star formation in half of massive galaxies was quenched by the time the Universe was 3
billion years old. Very low amounts of molecular gas seem to be responsible for this, at least …