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 …

Quasars at cosmic dawn provide powerful probes of the formation and growth of the earliest
supermassive black holes (SMBHs) in the Universe, their connections to galaxy and …

Context. LBQS 0302− 0019 is a blue quasar (QSO) at z∼ 3.3 that hosts powerful outflows
and resides in a complex environment consisting of an obscured active galactic nucleus …

We report the first plausible optical electromagnetic counterpart to a (candidate) binary black
hole merger. Detected by the Zwicky Transient Facility, the electromagnetic flare is …

We present the first results from the Map** Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …

Context. The AGN bolometric correction is a key element for understanding black hole (BH)
demographics and computing accurate BH accretion histories from AGN luminosities …

Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …

In this paper, we provide updated constraints on the bolometric quasar luminosity function
(QLF) from z= 0 to z= 7. The constraints are based on an observational compilation that …

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 …

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