Observations that resolve nearby galaxies into individual regions across multiple phases of
the gas–star formation feedback “matter cycle” have provided a sharp new view of molecular …

We present PHANGS–ALMA, the first survey to map CO J= 2→ 1 line emission at∼ 1''∼ 100
pc spatial resolution from a representative sample of 90 nearby (d≲ 20 Mpc) galaxies that lie …

We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field
spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …

Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …

Using a compilation of 25 studies from the literature, we investigate the evolution of the star-
forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out …

We measure the star formation efficiency (SFE), the star formation rate (SFR) per unit of gas,
in 23 nearby galaxies and compare it with expectations from proposed star formation laws …

We present a comprehensive analysis of the relationship between star formation rate
surface density, Σ SFR, and gas surface density, Σ gas, at sub-kpc resolution in a sample of …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …

Using free–free emission measured in the Ka band (26–40 GHz) for 10 star-forming regions
in the nearby galaxy NGC 6946, including its starbursting nucleus, we compare a number of …

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 …