Compact steep-spectrum (CSS) and peaked-spectrum (PS) radio sources are compact,
powerful radio sources. The multi-frequency observational properties and current theories …

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 …

It remains a major challenge to derive a theory of cloud-scale (pc) star formation and
feedback, describing how galaxies convert gas into stars as a function of the galactic …

We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …

The Sloan Digital Sky Survey (SDSS) has been observing the universe using the 2.5 m
Sloan Foundation Telescope (Gunn et al. 2006) at Apache Point Observatory (APO) for over …

It is a major open question which physical processes stop gas accretion on to giant
molecular clouds (GMCs) and limit the efficiency at which gas is converted into stars. While …

We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in
the mean atomic and molecular gas mass fractions throughout the SFR–M* plane and along …

We present an atlas of 129 spectral energy distributions for nearby galaxies, with
wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a …

Abstract We present the Lambda Adaptive Multi-Band Deblending Algorithm in R (lambdar),
a novel code for calculating matched aperture photometry across images that are neither …

ABSTRACT The Galaxy And Mass Assembly (GAMA) survey furnishes a deep redshift
catalog that, when combined with the Wide-field Infrared Survey Explorer (WISE), allows us …