The new capabilities that JWST offers in the near-and mid-infrared (IR) are used to
investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources …

We present the implications for cosmic inflation of the Planck measurements of the cosmic
microwave background (CMB) anisotropies in both temperature and polarization based on …

The evolution of the number density of galaxies in the universe, and thus also the total
number of galaxies, is a fundamental question with implications for a host of astrophysical …

Using data from the COSMOS survey, we perform the first joint analysis of galaxy–galaxy
weak lensing, galaxy spatial clustering, and galaxy number densities. Carefully accounting …

Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and
Quiescent Galaxies - IOPscience This site uses cookies. By continuing to use this site you …

We study a new population of extremely red objects (EROs) recently discovered by the
James Webb Space Telescope (JWST) based on their NIRCam colors F277W− F444W> 1.5 …

We show that measures of star formation rates (SFRs) for infrared galaxies using either
single-band 24 μm or extinction-corrected Paα luminosities are consistent in the total …

We study the relation between molecular gas and star formation in a volume-limited sample
of 222 galaxies from the COLD GASS survey, with measurements of the CO (1–0) line from …

We use a suite of semi-empirical models to predict the galaxy–galaxy merger rate and
relative contributions to bulge growth as a function of mass (both halo and stellar), redshift …

We present spatially resolved Atacama Large Millimeter/submillimeter Array (ALMA) 870 μm
dust continuum maps of six massive, compact, dusty star-forming galaxies at z∼ 2.5. These …