collaborators

5 papers

astro-ph.GA2026

On the later evolution of observationally selected protocluster candidates at

Seunghwan Lim

Recent observations have revealed numerous protocluster candidates at , yet whether these systems will eventually evolve into today's galaxy clusters remains an op…

astro-ph.GA2026

Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe

Callum Witten, Jake S. Bennett, Pascal A. Oesch +8

JWST has revealed an overabundance of apparent (`Coma'-like) cluster progenitors at that is two (300) times in excess of, and in () tension with, the numb…

astro-ph.GA2025

Think inside the box: cosmic variance and large-scale conformity of high-redshift massive galaxies in the FLAMINGO simulations

Seunghwan Lim, Sandro Tacchella, Roberto Maiolino +2

We use the highest-resolution FLAMINGO hydrodynamical simulation to quantify cosmic variance and large-scale coherence in the evolution of massive galaxies at high redshift. FLAMIN…

astro-ph.GA2025

In-situ vs. ex-situ drivers of galaxy quenching: critical black hole mass and main sequence universality in the FLAMINGO simulation

Seunghwan Lim, Sandro Tacchella, Roberto Maiolino +2

Exploiting a large sample of 5.3 million galaxies with from the highest-resolution FLAMINGO simulation, we carry out a statistical analysis…

astro-ph.GA2025

The abundance and nature of high-redshift quiescent galaxies from JADES spectroscopy and the FLAMINGO simulations

William M. Baker, Seunghwan Lim, Francesco D'Eugenio +20

We use NIRSpec/MSA spectroscopy and NIRCam imaging to study a sample of 18 massive (dex), central quiescent galaxies at in the GOO…