activity
20172024
most citedThe erratic dynamical life of black hole seeds in high-redshift galaxies

135 citations · 774 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2024★ 17 cited

Rates of Stellar Tidal Disruption Events around Intermediate-Mass Black Holes

Janet N. Y. Chang, Lixin Dai, Hugo Pfister +2

Rates of stellar tidal disruption events (TDEs) around supermassive black holes (SMBHs) have been extensively calculated using the loss cone theory, while theoretical work on TDE r…

astro-ph.HE2022★ 1 cited

A fast rising tidal disruption event from a candidate intermediate mass black hole

C. R. Angus, V. F. Baldassare, B. Mockler +36

Massive black holes (BHs) at the centres of massive galaxies are ubiquitous. The population of BHs within dwarf galaxies, on the other hand, is evasive. Dwarf galaxies are thought…

gr-qc2022★ 6 cited

Astrophysics with the Laser Interferometer Space Antenna

Pau Amaro Seoane, Jeff Andrews, Manuel Arca Sedda +156

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 many…

astro-ph.GA2021

Dual AGN in the Horizon-AGN simulation and their link to galaxy and massive black hole mergers, with an excursus on multiple AGN

Marta Volonteri, Hugo Pfister, Ricarda Beckmann +5

The occurrence of dual active galactic nuclei (AGN) on scales of a few tens of kpc can be used to study merger-induced accretion on massive black holes (MBHs) and to derive clues o…

astro-ph.HE2021★ 20 cited

Revisiting the Rates and Demographics of Tidal Disruption Events: Effects of the Disk Formation Efficiency

Thomas Hong Tsun Wong, Hugo Pfister, Lixin Dai

Tidal disruption events (TDEs) are valuable probes of the demographics of supermassive black holes as well as the dynamics and population of stars in the centers of galaxies. In th…

astro-ph.GA2021★ 12 cited

Supernova-driven turbulent metal mixing in high redshift galactic disks: metallicity fluctuations in the interstellar medium and its imprints on metal poor stars in the Milky Way

Anne Noer Kolborg, Davide Martizzi, Enrico Ramirez-Ruiz +4

The extent to which turbulence mixes gas in the face of recurrent infusions of fresh metals by supernovae (SN) could help provide important constraints on the local star formation…

astro-ph.SR2021★ 67 cited

The Early Phases of Supernova 2020pni: Shock-Ionization of the Nitrogen-Enriched Circumstellar Material

G. Terreran, W. V. Jacobson-Galan, J. H. Groh +20

We present multiwavelength observations of the Type II SN 2020pni. Classified at days after explosion, the object showed narrow (FWHM $<250\,\textrm{km}\,\textrm{s}^{-1}…

astro-ph.HE2021★ 24 cited

Observable gravitational waves from tidal disruption events and their electromagnetic counterpart

Hugo Pfister, Martina Toscani, Thomas Hong Tsun Wong +3

We estimate the rate of tidal disruption events (TDEs) that will be detectable with future gravitational wave detectors as well as the most probable properties of these events and…

astro-ph.HE2020★ 106 cited

The Young Supernova Experiment: Survey Goals, Overview, and Operations

D. O. Jones, R. J. Foley, G. Narayan +68

Time domain science has undergone a revolution over the past decade, with tens of thousands of new supernovae (SNe) discovered each year. However, several observational domains, in…

astro-ph.GA2020★ 28 cited

Tidal disruption events in the first billion years of a galaxy

Hugo Pfister, Jane Dai, Marta Volonteri +3

Accretion of stars on massive black holes (MBHs) can feed MBHs and generate tidal disruption events (TDEs). We introduce a new physically motivated model to self-consistently treat…

astro-ph.GA2020★ 123 cited

Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations

Marta Volonteri, Hugo Pfister, Ricarda S. Beckman +12

Massive black hole (MBH) coalescences are powerful sources of low-frequency gravitational waves. To study these events in the cosmological context we need to trace the large-scale…

astro-ph.GA2020★ 49 cited

Enhancement of the tidal disruption event rate in galaxies with a nuclear star cluster: from dwarfs to ellipticals

Hugo Pfister, Marta Volonteri, Jane Lixin Dai +1

We compute the tidal disruption event (TDE) rate around local massive black holes (MBHs) with masses as low as , thus probing the dwarf regime for the…

astro-ph.GA2020★ 97 cited

The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters

Maxime Trebitsch, Yohan Dubois, Marta Volonteri +9

We present the Obelisk project, a cosmological radiation-hydrodynamics simulation following the assembly and reionization of a protocluster progenitor during the first two billions…

astro-ph.GA2020★ 8 cited

Real galaxy mergers from galaxy pair catalogs

Hugo Pfister, Massimo Dotti, Clothilde Laigle +2

Mergers of galaxies are extremely violent events shaping their evolution. Such events are thought to trigger starbursts and, possibly, black hole accretion. Nonetheless, it is stil…

astro-ph.GA2019★ 24 cited

Tidal disruption event rates in galaxy merger remnants

Hugo Pfister, Ben Bar-Or, Marta Volonteri +2

The rate of tidal disruption events (TDEs) depends sensitively on the stellar properties of the central galactic regions. Simulations show that galaxy mergers cause gas inflows, tr…

astro-ph.GA2019★ 135 cited

The erratic dynamical life of black hole seeds in high-redshift galaxies

Hugo Pfister, Marta Volonteri, Yohan Dubois +2

The dynamics of black hole seeds in high redshift galaxies is key to understand their ability to grow via accretion and to pair in close binaries during galactic mergers. To proper…

astro-ph.GA2017★ 57 cited

The birth of a supermassive black hole binary

Hugo Pfister, Alessandro Lupi, Pedro R. Capelo +3

We study the dynamical evolution of supermassive black holes, in the late stage of galaxy mergers, from kpc to pc scales. In particular, we capture the formation of the binary, a n…