Radio jets and the lobes they inflate are common in cool-core clusters and are known to play
a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is …

Galaxies are observed to host magnetic fields with a typical total strength of around 15 μ G.
A coherent large-scale field constitutes up to a few microgauss of the total, while the rest is …

Constraining the escape fraction of Lyman Continuum (LyC) photons from high-redshift
galaxies is crucial to understanding reionization. Recent observations have demonstrated …

During the epoch of reionization, the first galaxies were enshrouded in pristine neutral gas,
with one of the brightest emission lines in star-forming galaxies, Lyman α (Lyα), expected to …

Lyα emission is an exceptionally informative tracer of the life cycle of evolving galaxies and
the escape of ionizing photons. However, theoretical studies of Lyα emission are often …

We study star formation variability, or burstiness, as a method to constrain and compare
different galaxy formation models at high redshift using the azahar simulation suite. The …

The circumgalactic medium (CGM) contains information on the cumulative effect of galactic
outflows over time, generally thought to be caused by feedback from star formation and …

During the last decade, cosmological simulations have managed to reproduce realistic and
morphologically diverse galaxies, spanning the Hubble sequence. Central to this success …

We present a novel approach to extracting dwarf galaxies from photometric data to measure
their average halo mass profile with weak lensing. We characterize their stellar mass and …

We present SPICE, a new suite of radiation-hydrodynamic, cosmological simulations
targeting the epoch of reionization. The goal of these simulations is to systematically probe a …