Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

We present a set of multiwavelength mosaics and photometric catalogs in the Atacama
Large Millimeter/submillimeter Array (ALMA) lensing cluster survey fields. The catalogs were …

HDF850. 1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known
as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at …

Abstract Using the novel James Webb Space Telescope (JWST)/NIRCam observations in
the A2744 field, we present a first spatially resolved overview of a Hubble Space Telescope …

Recent data from the James Webb Space Telescope allow a first glimpse of galaxies at z≳
11. The most successful tool for identifying ultra-high-redshift candidates and inferring their …

Recent works have suggested that energy balance spectral energy distribution (SED) fitting
codes may be of limited use for studying high-redshift galaxies for which the observed …

Using NOEMA and ALMA 3mm line scans, we measured spectroscopic redshifts of six new
dusty galaxies at 3.5< z< 4.2 by solidly detecting [CI](1-0) and CO transitions. The sample …

To understand the active galactic nuclei (AGNs) phenomenon and their impact on the
evolution of galaxies, a complete AGN census is required; however, finding heavily …

Aims. This work aims to determine how the galaxy main sequence (MS) changes using
seven different commonly used methods to select the star-forming galaxies within VIPERS …