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 …

70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

We study the population of supermassive black holes (SMBHs) and their effects on massive
central galaxies in the IllustrisTNG cosmological hydrodynamical simulations of galaxy …

We present results from the" Mint" resolution DC Justice League suite of Milky Way–like
zoom-in cosmological simulations, which extend our study of nearby galaxies down into the …

Pulsar timing array (PTA) collaborations in North America, Australia, and Europe, have been
exploiting the exquisite timing precision of millisecond pulsars over decades of observations …

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 …

The origin and properties of the initial black hole seeds that grow to produce the observed
population of accreting sources remain to be determined. It is a challenge to uniquely …

In this paper, we provide predictions for the black hole (BH) population that would be
observable with planned JWST surveys at 5≤ z≤ 15. We base our study on the recently …

Coalescing massive black hole binaries (MBHBs) of, forming in the aftermath of galaxy
mergers, are primary targets of the space mission LISA, the Laser Interferometer Space …

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 …