15 citations · 18 across the 4 of their papers we have counts for
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astro-ph.GA2026
A Dusty Quenching-candidate AGN host at z=5.7: massive quiescent galaxies may quench already during the dust-obscured phase
Francesco D'Eugenio, Matilde Brazzini, Roberto Maiolino +12
We present a spectro-photometric analysis of RUBIES-EGS-9809, a broad-line AGN host at z=5.7 with a Balmer break and a dominant point source. The source is dust reddened (3 m…
astro-ph.GA2024★ 1 cited
The Astrid Simulation: Evolution of black holes and galaxies to z=0.5 and different evolution pathways for galaxy quenching
Yueying Ni, Nianyi Chen, Yihao Zhou +5
We present new results from the ASTRID simulation from to , covering the epoch of cosmic noon. The galaxy stellar mass function, as well as the black hole mass and lum…
astro-ph.GA2024★ 15 cited
Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at : A Comparative Study With IllustrisTNG and ASTRID
Emma Jane Weller, Fabio Pacucci, Yueying Ni +2
Recent JWST observations have uncovered an unexpectedly large population of massive quiescent galaxies at . Using the cosmological simulations IllustrisTNG and ASTRID, we iden…