Radio galaxies and feedback from AGN jets
We review current understanding of the population of radio galaxies and radio-loud quasars
from an observational perspective, focusing on their large-scale structures and dynamics …
from an observational perspective, focusing on their large-scale structures and dynamics …
The quest for dual and binary supermassive black holes: A multi-messenger view
The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …
Introducing the thesan project: radiation-magnetohydrodynamic simulations of the epoch of reionization
We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …
simulations that simultaneously model the large-scale statistical properties of the …
simba: Cosmological simulations with black hole growth and feedback
We introduce the simba simulations, the next generation of the mufasa cosmological galaxy
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
The IllustrisTNG simulations: public data release
We present the full public release of all data from the TNG100 and TNG300 simulations of
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …
First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
We have generated synthetic images of∼ 27 000 galaxies from the IllustrisTNG and the
original Illustris hydrodynamic cosmological simulations, designed to match Pan-STARRS …
original Illustris hydrodynamic cosmological simulations, designed to match Pan-STARRS …
The ASTRID simulation: the evolution of supermassive black holes
We present the evolution of black holes (BHs) and their relationship with their host galaxies
in Astrid, a large-volume cosmological hydrodynamical simulation with box size 250 h …
in Astrid, a large-volume cosmological hydrodynamical simulation with box size 250 h …
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback
In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …