JWST has detected many overmassive galactic systems at z> 4, where the mass of the black
hole, M•, is 10–100 times larger than expected from local relations, given the host's stellar …

Growing supermassive black holes (Active Galactic Nuclei; AGN) release energy with the
potential to alter their host galaxies and larger-scale environment; a process named “AGN …

Many quiescent galaxies discovered in the early Universe by JWST raise fundamental
questions on when and how these galaxies became and stayed quenched. Making use of …

The nucleus of almost all massive galaxies contains a supermassive black hole (BH). The
feedback from the accretion of these BHs is often considered to have crucial roles in …

One of the most important questions in astrophysics is what causes galaxies to stop forming
stars. Previous studies have shown a tight link between quiescence and black hole mass …

We present an analysis of the quenching of local observed and simulated galaxies,
including an investigation of the dependence of quiescence on both intrinsic and …

We present the analysis of three intermediate-mass quiescent galaxies (QGs) with stellar
masses of∼ 1010 M⊙ at redshifts z∼ 3–4 using NIRSpec low-resolution spectroscopy …

We measure the broad impact of galaxy structure on galaxy formation by examining the
ongoing star formation and integrated star formation history as revealed through the stellar …

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 …

We explore the co-evolution of dark matter halos, their central galaxies, and central
supermassive black holes (SMBHs) using the IllustrisTNG (TNG) simulation. We find that the …