JWST is revolutionizing our understanding of the high-z Universe by expanding the black
hole horizon, looking farther and to smaller masses, and revealing the stellar light of their …

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

The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …

We review the properties of the established Scaling Relations (SRs) of galaxies and active
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …

Active galactic nuclei (AGNs) in dwarf galaxies could host the relics of those early universe
seed black holes that did not grow into supermassive black holes. Using MaNGA integral …

We present measurements of broad emission lines and virial estimates of supermassive
black hole masses (M BH) for a large sample of ultrahard X-ray-selected active galactic …

We determine the low-redshift X-ray luminosity function, active black hole mass function
(BHMF), and Eddington ratio distribution function (ERDF) for both unobscured (Type 1) and …

Context. Sources at the brightest end of the quasi-stellar object (QSO) luminosity function,
during the peak epoch in the history of star formation and black hole accretion (z∼ 2− 4 …

We present new central stellar velocity dispersions for 484 Sy 1.9 and Sy 2 from the second
data release of the Swift/BAT AGN Spectroscopic Survey (BASS DR2). This constitutes the …

We present new near-infrared VLTI/GRAVITY interferometric spectra that spatially resolve
the broad Brγ emission line in the nucleus of the active galaxy IRAS 09149− 6206. We use …