The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for
gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key …

The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological
focus: to probe the expansion rate of the universe, and to understand stochastic …

Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is
a consensus that galaxies emerged from the expanding matter background by gravitational …

We present a reduction and analysis of the James Webb Space Telescope (JWST) SMACS
0723 field using new post-launch calibrations to conduct a search for ultra-high-redshift …

We present release 1.3 of the ALPS (Algorithms and Libraries for Physics Simulations)
project, an international open-source software project to develop libraries and application …

Over the past decades, rest-frame ultraviolet (UV) observations have provided large samples
of UV luminous galaxies at redshift (z) greater than 6 (refs. ), during the so-called epoch of …

The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large
Program (LP) that is identifying and performing a first characterization of many of the most …

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic
model of galaxy formation to explain the dust content of 13 Lyman break galaxies (LBGs) …

ALMA observations have revealed the presence of dust in the first generations of galaxies in
the Universe. However, the dust temperature T d remains mostly unconstrained due to the …

… , where we do expect dust extinction to be more severe (Dayal et al. 2022; Sommovigo et
al. 2022). … form, successfully tested on a wide redshift range, proposed by Dayal et al. (2014): …