activity
20222026
most citedThe low-end of the black hole mass function at cosmic dawn

101 citations · 381 across the 24 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2026

A tidal disruption event in a quasar at redshift 7.19

S. Fujimoto, Q. Fei, G. B. Brammer +41

We report a long-lived nuclear transient in GNz7q, a red quasar at powered by a black hole and hosted by a compact, dusty starburst galaxy. Th…

astro-ph.GA2026

How can we finally see the first light? Status and perspective in the search for Population III stars

Alessandra Venditti, Daniel Schaerer, Erik Zackrisson +26

Finding the first (Population III or Pop III) stars is one of the fundamental quests of astronomy, aiming to deliver the missing link in how stars form at early cosmic times. Yet t…

astro-ph.GA2026

The role of major mergers in triggering super-Eddington accretion

Riccardo Caleno, Tommaso Zana, Raffaella Schneider +6

JWST observations have opened a new era in the exploration of the high-redshift Universe, revealing black holes (BHs) with masses of several million solar masses already at ,…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…

astro-ph.GA2026

Gravitational Waves from Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA, and LISA

Nazanin Davari, Rosa Valiante, Alessandro Trinca +8

Next-generation detectors, such as LISA, LGWA, and ET, will for the first time probe the high redshift Universe, offering unique insight into the birth, growth, and dynamics of the…

astro-ph.GA2026★ 1 cited

You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei

Alessandro Trinca, Alessandro Lupi, Francesco Haardt +1

We revisit black hole mass estimates for high-redshift broad-line active galactic nuclei (AGNs) discovered with JWST by jointly analysing their broad emission lines and their syste…

astro-ph.GA2026

Too many or too massive? Investigating the high- demography of active SMBHs from JWST

Daniel Roberts, Francesco Shankar, Vieri Cammelli +12

Recent JWST observations have unveiled a numerous population of low-luminosity active galactic nuclei (AGN) at , with space densities roughly an order of magnitude above p…

astro-ph.GA2026★ 1 cited

Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars

Alessandro Trinca, Alessandro Lupi, Zoltán Haiman +4

The rapid emergence of supermassive black holes (SMBHs) in the early Universe poses a challenge to current models of black hole growth. One promising formation pathway is the direc…

astro-ph.GA2025

BlackTHUNDER: Evidence of three massive black holes in a z~5 galaxy

Hannah Übler, Giovanni Mazzolari, Roberto Maiolino +41

We present observational evidence of three massive, accreting black holes (BHs) in the z=5.0167 galaxy J0148-4214 from JWST/NIRSpec-IFU spectroscopy. The BHs are revealed through b…

astro-ph.GA2025★ 17 cited

A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization

Ignas Juodžbalis, Cosimo Marconcini, Francesco D'Eugenio +37

Recent discoveries of faint active galactic nuclei (AGN) at the redshift frontier have revealed a plethora of broad \Halpha emitters with optically red continua, named Little Red D…

astro-ph.GA2025★ 2 cited

Super-Eddington accretion in protogalactic cores

Tommaso Zana, Pedro R. Capelo, Mairo Boresta +6

The presence of massive black holes (BHs) exceeding already at redshift challenges standard models of BH growth. Super-Eddington (SE) accretion has…

astro-ph.GA2025★ 11 cited

JADES reveals a large population of low mass black holes at high redshift

Sophia Geris, Roberto Maiolino, Yuki Isobe +24

JWST has revealed a large population of active galactic nuclei (AGN) in the distant universe, which are challenging our understanding of early massive black hole seeding and growth…

astro-ph.GA2025★ 27 cited

A black hole in a near-pristine galaxy 700 million years after the Big Bang

Roberto Maiolino, Hannah Uebler, Francesco D'Eugenio +36

The recent discovery of a large number of massive black holes within the first two billion years after the Big Bang, as well as their peculiar properties, have been largely unexpec…

astro-ph.GA2025★ 2 cited

Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots

Giada Quadri, Alessandro Trinca, Alessandro Lupi +2

The advent of the James Webb Space Telescope has revolutionised our understanding of the high-redshift Universe through its detection of bright, massive galaxies up to $z\gtrsim 10…

astro-ph.GA2025★ 13 cited

Pushing JWST to the extremes: search and scrutiny of bright galaxy candidates at z15-30

M. Castellano, A. Fontana, E. Merlin +50

We designed customized Lyman-break color selection techniques to identify galaxy candidates in the redshift ranges and . The selection was pe…

astro-ph.CO2025★ 8 cited

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Hannah O'Brennan, John A. Regan, John Brennan +5

The recent detections of a large number of candidate active galactic nuclei at high redshift (i.e. ) has increased speculation that heavy seed massive black hole forma…

astro-ph.GA2025★ 7 cited

BlackTHUNDER -- A non-stellar Balmer break in a black hole-dominated little red dot at

Xihan Ji, Roberto Maiolino, Hannah Übler +34

Recent observations from JWST have revealed an abundant population of active galactic nuclei (AGN) and so-called ``Little Red Dots'' (LRDs) at , many of wh…

astro-ph.GA2024★ 8 cited

Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe

Alessandro Trinca, Rosa Valiante, Raffaella Schneider +7

Early JWST observations are providing growing evidence for a ubiquitous population of accreting supermassive black holes (BHs) at high redshift, many of which appear overmassive co…

astro-ph.GA2024★ 93 cited

A dormant, overmassive black hole in the early Universe

Ignas Juodžbalis, Roberto Maiolino, William M. Baker +25

Recent observations have found a large number of supermassive black holes already in place in the first few hundred million years after Big Bang. The channels of formation and grow…

astro-ph.HE2023

Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Stephen Fairhurst, Cameron Mills, Monica Colpi +4

We investigate the detectability of single-event coalescing black hole binaries with total mass of at cosmological distances () with t…

astro-ph.GA2023★ 3 cited

Are we surprised to find SMBHs with JWST at z > 9?

Raffaella Schneider, Rosa Valiante, Alessandro Trinca +3

JWST is unveiling for the first time accreting black holes (BHs) with masses of 10^6 - 10^7 Msun at z > 4, with the most distant residing in GNz11 at z = 10.6. Are we really surpri…

astro-ph.GA2023★ 8 cited

Exploring the nature of UV-bright galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?

Alessandro Trinca, Raffaella Schneider, Rosa Valiante +4

We use the Cosmic Archaeology Tool (CAT) semi-analytical model to explore the contribution of Population (Pop) III/II stars and active galactic nuclei (AGNs) to the galaxy UV lumin…

astro-ph.GA2023★ 17 cited

Direct-collapse black hole formation induced by internal radiation of host halos

Gen Chiaki, Sunmyon Chon, Kazuyuki Omukai +3

We estimate the fraction of halos that host supermassive black holes (SMBHs) forming through the direct collapse (DC) scenario by using cosmological N -body simulations combined wi…

astro-ph.GA2022★ 43 cited

Seeking the growth of the first black hole seeds with JWST

Alessandro Trinca, Raffaella Schneider, Roberto Maiolino +3

In this paper we provide predictions for the BH population that would be observable with planned JWST surveys at . We base our study on the recently developed Cosmi…