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 …

This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …

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 …

We compare molecular gas traced by 12 CO (2–1) maps from the HERACLES survey, with
tracers of the recent star formation rate (SFR) across 30 nearby disk galaxies. We …

We use a newly assembled sample of 3545 star-forming galaxies with secure spectroscopic,
grism, and photometric redshifts at z= 1.5–2.5 to constrain the relationship between UV …

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 …

Aims. The goal of this paper is to analyse the behaviour of the gas-to-dust mass ratio (G/D)
of local Universe galaxies over a wide metallicity range. We especially focus on the low …

We estimate the conversion factor relating CO emission to H 2 mass, α CO, in five Local
Group galaxies that span approximately an order of magnitude in metallicity—M 31, M 33 …

The total star formation budget of galaxies consists of the sum of the unobscured star
formation, as observed in the rest-frame ultraviolet (UV), together with the obscured …

ABSTRACT The KINGFISH project (Key Insights on Nearby Galaxies: a Far-Infrared Survey
with Herschel) is an imaging and spectroscopic survey of 61 nearby (d< 30 Mpc) galaxies …