In our modern understanding of galaxy formation, every galaxy forms within a dark matter
halo. The formation and growth of galaxies over time is connected to the growth of the halos …

Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …

One of the key open questions in extragalactic astronomy is what stops star formation in
galaxies. While it is clear that the cold gas reservoir, which fuels the formation of new stars …

The tight correlations between the masses of supermassive black holes (BHs) and the
properties of their host galaxies suggest that BHs co-evolve with galaxies. However, what is …

Abstract The One-Percent survey of the Dark Energy Spectroscopic Instrument collected∼
270k emission line galaxies (ELGs) at 0.8< z< 1.6. The high completeness of the sample …

We have updated the Munich galaxy formation model to the Planck first-year cosmology,
while modifying the treatment of baryonic processes to reproduce recent data on the …

We explore three sets of cosmological hydrodynamical simulations, IllustrisTNG (TNG50,
TNG100, and TNG300), EAGLE, and SIMBA, to investigate the physical processes impacting …

Satellite galaxies in groups and clusters are more likely to have low star formation rates
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …

The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …

We measure the luminosity and color dependence of galaxy clustering in the largest-ever
galaxy redshift survey, the main galaxy sample of the Sloan Digital Sky Survey Seventh Data …