Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

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 …

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 …

We present the full public release of all data from the Illustris simulation project. Illustris is a
suite of large volume, cosmological hydrodynamical simulations run with the moving-mesh …

The next two decades are expected to open the door to the first coincident detections of
electromagnetic (EM) and gravitational-wave (GW) signatures associated with massive …

We investigate black hole–host galaxy scaling relations in cosmological simulations with a
self-consistent black hole growth and feedback model. Our sub-grid accretion model …

Gravitational waves (GWs) have now been detected from stellar-mass black hole binaries,
and the first observations of GWs from massive black hole (MBH) binaries are expected …

Recent discoveries of massive black holes (MBHs) in dwarf galaxies suggest that they may
have a more common presence than once thought. Systematic searches are revealing more …

We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …

We characterize the population of wandering black holes, defined as those physically offset
from their halo centres, in the romulus cosmological simulations. Unlike most other currently …