There is growing observational evidence for dwarf galaxies hosting active galactic nuclei
(AGN), including hints of AGN-driven outflows in dwarfs. However, in the common theoretical …

We analyse the quenched fractions, gas content, and star formation histories of∼ 1200
satellite galaxies with M*≥ 5× 106 M⊙ around 198 Milky Way-(MW) and Andromeda-like …

We examine the properties of the low-redshift circumgalactic medium (CGM) around star-
forming and quenched galaxies in the simba cosmological hydrodynamic simulations …

We study the star formation history (SFH) of the ultradiffuse galaxy (UDG) Dragonfly 44
(DF44) based on the simultaneous fit to near-ultraviolet to near-infrared photometry and high …

We apply the radiative transfer (RT) code skirt on a sample of low-redshift (z≤ 0.1) galaxies
extracted from the TNG50 simulation to enable an apples-to-apples comparison with …

Recent systematic searches for massive black holes (BHs) in local dwarf galaxies led to the
discovery of a population of faint active galactic nuclei (AGNs). We investigate the …

We explore the characteristics of actively accreting massive black holes (MBHs) within dwarf
galaxies in the R omulus25 cosmological hydrodynamic simulation. We examine the MBH …

The-to-UV luminosity ratio () is often used to probe bursty star formation histories (SFHs) of
star-forming galaxies and it is important to validate it against other proxies for burstiness. To …

Abstract The PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) catalog will
provide measurements of galaxy properties, such as stellar mass (M*), star formation rate …

A debate is emerging regarding the recent inconsistent results of different studies for the
cosmic star formation rate density (CSFRD) at high-z. We employ UV and IR data sets to …