activity
20002026
most citedLaser Interferometer Space Antenna

1.4k citations · 25.3k across the 283 of their papers we have counts for

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43 papers · 1 filter

astro-ph.CO2024

Large-scale dual AGN in large-scale cosmological hydrodynamical simulations

Clara Puerto-Sánchez, Melanie Habouzit, Marta Volonteri +10

Detecting dual active galactic nuclei (DAGN) in observations and understanding theoretically which massive black holes (MBHs) compose them and in which galactic and large-scale env…

astro-ph.CO2024★ 12 cited

Dark Matter Mounds: towards a realistic description of dark matter overdensities around black holes

Gianfranco Bertone, A. Renske A. C. Wierda, Daniele Gaggero +3

Dark matter overdensities around black holes can be searched for by looking at the characteristic imprint they leave on the gravitational waveform of binary black hole mergers. Cur…

astro-ph.CO2024★ 45 cited

LISA Definition Study Report

Monica Colpi, Karsten Danzmann, Martin Hewitson +108

The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…

astro-ph.CO2022★ 359 cited

Cosmology with the Laser Interferometer Space Antenna

Pierre Auclair, David Bacon, Tessa Baker +177

The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…

astro-ph.CO2015★ 50 cited

Assessing inflow rates in atomic cooling halos: implications for direct collapse black holes

M. A. Latif, M. Volonteri

Supermassive black holes are not only common in the present-day galaxies, but billion solar masses black holes also powered quasars. One efficient way to form such black…

astro-ph.CO2014★ 888 cited

Dancing in the dark: galactic properties trace spin swings along the cosmic web

Yohan Dubois, Christophe Pichon, Charlotte Welker +30

A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. Th…

astro-ph.CO2013★ 60 cited

New observational Constraints on the Growth of the First Supermassive Black Holes

E. Treister, K. Schawinski, M. Volonteri +1

We constrain the total accreted mass density in supermassive black holes at z>6, inferred via the upper limit derived from the integrated X-ray emission from a sample of photometri…

astro-ph.CO2013★ 65 cited

Nuclear coups: dynamics of black holes in galaxy mergers

Sandor Van Wassenhove, Pedro R. Capelo, Marta Volonteri +4

We study the dynamical evolution of supermassive black holes (BHs) in merging galaxies on scales of hundreds of kpc to 10 pc, to identify the physical processes that aid or hinder…

astro-ph.CO2013★ 39 cited

The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes

Jillian Bellovary, Alyson Brooks, Marta Volonteri +3

Using a set of zoomed-in cosmological simulations of high-redshift progenitors of massive galaxies, we isolate and trace the history of gas that is accreted by central supermassive…

astro-ph.CO2013★ 63 cited

The role of relativistic jets in the heaviest and most active supermassive black holes at high redshift

G. Ghisellini, F. Haardt, R. Della Ceca +2

In powerful radio-quiet active galactic nuclei (AGN), black holes heavier than one billion solar masses form at a redshift ~1.5-2. Supermassive black holes in jetted radio-loud AGN…

astro-ph.CO2013★ 167 cited

Black hole evolution: III. Statistical properties of mass growth and spin evolution using large-scale hydrodynamical cosmological simulations

Yohan Dubois, Marta Volonteri, Joseph Silk

Supermassive black holes (BH) at the centres of galaxies can rapidly change their mass and spin by gas accretion and mergers. Using hydrodynamical cosmological simulations, with pr…

astro-ph.CO2012★ 133 cited

On the orientation and magnitude of the black hole spin in galactic nuclei

M. Dotti, M. Colpi, S. Pallini +2

Massive black holes in galactic nuclei vary their mass M and spin vector J due to accretion. In this study we relax, for the first time, the assumption that accretion can be either…

astro-ph.CO2012★ 38 cited

Massive black holes in central cluster galaxies

Marta Volonteri, Luca Ciotti

We explore how the co-evolution of massive black holes (MBHs) and galaxies is affected by environmental effects, addressing in particular MBHs hosted in the central galaxies of clu…

astro-ph.CO2012★ 91 cited

Black Holes in the Early Universe

Marta Volonteri, Jillian Bellovary

The existence of massive black holes was postulated in the sixties, when the first quasars were discovered. In the late nineties their reality was proven beyond doubt, in the Milky…

astro-ph.CO2012★ 3 cited

The first massive black holes

Marta Volonteri

I briefly outline recent theoretical developments on the formation of the first massive black holes (MBHs) that may grow into the population of MBHs powering quasars and inhabiting…

astro-ph.CO2012★ 51 cited

Limits on the high redshift growth of massive black holes

R. Salvaterra, F. Haardt, M. Volonteri +1

We place firm upper limits on the global accretion history of massive black holes at z>5 from the recently measured unresolved fraction of the cosmic X-ray background. The maximum…

astro-ph.CO2012★ 320 cited

The Formation and Evolution of Massive Black Holes

Marta Volonteri

The past 10 years have witnessed a change of perspective in the way astrophysicists think about massive black holes (MBHs), which are now considered to have a major role in the evo…

astro-ph.CO2012★ 116 cited

High-redshift formation and evolution of central massive objects II: The census of BH seeds

B. Devecchi, M. Volonteri, E. M. Rossi +2

We present results of simulations aimed at tracing the formation of nuclear star clusters (NCs) and black hole (BH) seeds, in a cosmological context. We focus on two mechanisms for…

astro-ph.CO2012★ 115 cited

eLISA: Astrophysics and cosmology in the millihertz regime

Pau Amaro-Seoane, Sofiane Aoudia, Stanislav Babak +27

This document introduces the exciting and fundamentally new science and astronomy that the European New Gravitational Wave Observatory (NGO) mission (derived from the previous LISA…

astro-ph.CO2011★ 179 cited

Observability of Dual Active Galactic Nuclei in Merging Galaxies

Sandor Van Wassenhove, Marta Volonteri, Lucio Mayer +3

Supermassive black holes (SMBHs) have been detected in the centers of most nearby massive galaxies. Galaxies today are the products of billions of years of galaxy mergers, but also…

astro-ph.CO2011★ 74 cited

Assessing the redshift evolution of massive black holes and their hosts

Marta Volonteri, Daniel P. Stark

Motivated by recent observational results that focus on high redshift black holes, we explore the effect of scatter and observational biases on the ability to recover the intrinsic…

astro-ph.CO2011★ 33 cited

The mass function of black holes at 1<z<4.5: comparison of models with observations

Priyamvada Natarajan, Marta Volonteri

In this paper, we compare the observationally derived black hole mass function (BHMF) of luminous broad-line quasars (BLQSOs) at 1<z<4.5 drawn from the Sloan Digital Sky Survey (SD…

astro-ph.CO2011★ 126 cited

Cosmography with strong lensing of LISA gravitational wave sources

M. Sereno, Ph. Jetzer, A. Sesana +1

LISA might detect gravitational waves from mergers of massive black hole binaries strongly lensed by intervening galaxies (Sereno et al. 2010). The detection of multiple gravitatio…

astro-ph.CO2011★ 110 cited

The First Massive Black Hole Seeds and Their Hosts

Jillian Bellovary, Marta Volonteri, Fabio Governato +3

We investigate the formation of the first massive black holes in high redshift galaxies, with the goal of providing insights to which galaxies do or do not host massive black holes…