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 …

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 …

We study the properties of massive, galactic-scale outflows of molecular gas and investigate
their impact on galaxy evolution. We present new IRAM PdBI CO (1–0) observations of local …

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 …

We measure the low-J CO line ratios R 21≡ CO (2–1)/CO (1–0), R 32≡ CO (3–2)/CO (2–1),
and R 31≡ CO (3–2)/CO (1–0) using whole-disk CO maps of nearby galaxies. We draw CO …

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

Aims. We investigate the fueling and the feedback of star formation and nuclear activity in
NGC 1068, a nearby (D= 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and …

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 present∼ kiloparsec spatial resolution maps of the CO-to-H 2 conversion factor (α CO)
and dust-to-gas ratio (DGR) in 26 nearby, star-forming galaxies. We have simultaneously …

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 …