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∼ …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

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 present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

We combine molecular gas masses inferred from CO emission in 500 star-forming galaxies
(SFGs) between z= 0 and 3, from the IRAM-COLDGASS, PHIBSS1/2, and other surveys, with …

We present PHIBSS, the IRAM Plateau de Bure high-z blue sequence CO 3–2 survey of the
molecular gas properties in massive, main-sequence star-forming galaxies (SFGs) near the …

The main sequence (MS) of star-forming (SF) galaxies plays a fundamental role in driving
galaxy evolution and our efforts to understand it. However, different studies find significant …

We explore star formation histories (SFHs) of galaxies based on the evolution of the star
formation rate stellar mass relation (SFR–M*). Using data from the FourStar Galaxy …

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) …

Two main modes of star formation are know to control the growth of galaxies: a relatively
steady one in disk-like galaxies, defining a tight star formation rate (SFR)–stellar mass …