Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …

Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-
metal ratio (DTM) from z= 0→ 6, using a model for the production, growth, and destruction of …

ABSTRACT The James Webb Space Telescope (JWST) promises to revolutionize our
understanding of the early Universe, and contrasting its upcoming observations with …

Dust-obscured star formation has dominated the cosmic history of star formation, since z≃ 4.
However, the recent finding of significant amount of dust in galaxies out to z≃ 8 has opened …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

Dust in galaxies is an important tracer of galaxy properties and their evolution over time. The
physical origin of the grain size distribution, the dust chemical composition, and, hence, the …

Contrary to many stereotypes about massive galaxies, observed brightest group galaxies
(BGGs) are diverse in their star formation rates, kinematic properties, and morphologies …