CO line emission represents the most accessible and widely used tracer of the molecular
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …

Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

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 …

Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …

Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …

Using data from the mid-infrared to millimeter wavelengths for individual galaxies and for
stacked ensembles at 0.5< z< 2, we derive robust estimates of dust masses (M dust) for main …

We report on the detection of the [C ii] 157.7 μ m emission from the Lyman break galaxy
(LBG) MACS0416_Y1 at z= 8.3113, by using the Atacama Large Millimeter/submillimeter …

Three billion years after the big bang (at redshift z= 2), half of the most massive galaxies
were already old, quiescent systems with little to no residual star formation and extremely …

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) …

Star-forming galaxies (SFGs) display a continuous specific star formation rate (sSFR)
distribution, which can be approximated by two log-normal functions: one encompassing the …