Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …

Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics …

We analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …

Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

Parametric models for galaxy star formation histories (SFHs) are widely used, though they
are known to impose strong priors on physical parameters. This has consequences for …

Galaxy observations are influenced by many physical parameters: stellar masses, star
formation rates (SFRs), star formation histories (SFHs), metallicities, dust, black hole activity …

We combine the recent determination of the evolution of the cosmic density of molecular gas
(H 2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar …

We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …

The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …