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 present an atlas of ultraviolet and infrared images of∼ 15,750 local (d≲ 50 Mpc)
galaxies, as observed by NASA's Wide-field Infrared Survey Explorer (WISE) and Galaxy …

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 …

We use spectral energy distribution fitting to place constraints on the stellar populations of
59 ultra-diffuse galaxies (UDGs) in the low-to-moderate density fields of the MATLAS survey …

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 …

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 present GLADE+, an extended version of the GLADE galaxy catalogue introduced in our
previous paper for multimessenger searches with advanced gravitational-wave detectors …