activity
20152026
most citedThe second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

1k citations · 2.6k across the 47 of their papers we have counts for

collaborators

50 papers

astro-ph.GA2026

Gas-induced gravitational-wave dephasing and accretion periodicities of live post-Newtonian massive black hole binaries: warm disk

Mudit Garg, Alessia Franchini, Alessandro Lupi

We perform 3D hydrodynamical simulations of an equal-mass quasi-circular live massive black hole binary (MBHB) embedded in a prograde, locally isothermal circu…

astro-ph.EP2026

Misaligned circumbinary discs around unequal-mass eccentric binaries: alignment, morphology, and binary accretion variability

Ruiqi Yang, Jeremy L. Smallwood, Hongping Deng +4

Binary systems are ubiquitous in the Universe and often host circumbinary discs that are misaligned with the binary orbital plane. Such misalignments can affect disc evolution and…

astro-ph.HE2026

Even a precessing clock is right twice per orbit -- The super-periods of eRO-QPE2 and challenges for quasi-periodic eruption orbital models

R. Arcodia, G. Miniutti, J. Chakraborty +25

We present OC (``observed minus calculated'') timing analysis of the quasi-periodic eruption (QPE) source eRO-QPE2 with a multi-mission X-ray campaign, which includes 32 observe…

astro-ph.HE2026

Spacetime in motion: an evolving relativistic binary black hole metric for GIZMO

Giacomo Fedrigo, Alessandro Lupi, Alessia Franchini +1

The last evolutionary stages of massive black hole binaries prior to coalescence is dominated by the emission of gravitational waves, which will be probed by the future Laser Inter…

astro-ph.HE2026

Large-amplitude modulations and hours-timescale variability in the early X-ray light curve of a tidal disruption flare

A. Malyali, A. Rau, P. Baldini +11

We present new X-ray, optical, and UV observations of the tidal disruption event candidate eRASSt J234402.9-352640, (hereafter J2344). Between 50 and 60 days after peak optical bri…

astro-ph.EP2024

Circumbinary accretion as a diagnostic for binary--disc misalignment

Jeremy L. Smallwood, Ya-Ping Li, Hongping Deng +1

Binary star systems can accrete material originating from a circumbinary disc. Since it is common for the circumbinary disc to be tilted with respect to the binary orbital plane, w…

astro-ph.CO2024

Searches for signatures of ultra-light axion dark matter in polarimetry data of the European Pulsar Timing Array

N. K. Porayko, P. Usynina, J. Terol-Calvo +74

Ultra-light axion-like particles (ALPs) can be a viable solution to the dark matter problem. The scalar field associated with ALPs, coupled to the electromagnetic field, acts as an…

astro-ph.HE2024

The fate of EMRI-IMRI pairs in AGN accretion disks: hydrodynamic and three body simulations

Peng Peng, Alessia Franchini, Matteo Bonetti +2

Extreme-mass-ratio inspirals (EMRIs) and intermediate-mass-ratio inspirals (IMRIs) are important gravitational wave (GW) sources for the Laser Interferometer Space Antenna (LISA).…

astro-ph.HE2024★ 18 cited

Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 069

Giovanni Miniutti, Alessia Franchini, Matteo Bonetti +8

X-ray quasi-periodic eruptions (QPEs) are intense soft X-ray bursts from the nuclei of nearby low-mass galaxies typically lasting about one hour and repeating every few. Their phys…

astro-ph.HE2024

Repeating transients in galactic nuclei: confronting observations with theory

Petra Suková, Francesco Tombesi, Dheeraj R. Pasham +5

In the last few years, a mysterious new class of astrophysical objects has been uncovered. These are spatially coincident with the nuclei of external galaxies and show X-ray variat…

astro-ph.HE2024★ 1 cited

Gas-induced perturbations on the gravitational wave in-spiral of live post-Newtonian LISA massive black hole binaries

Mudit Garg, Alessia Franchini, Alessandro Lupi +2

We investigate the effect of dynamically coupling gas torques with gravitational wave (GW) emission during the orbital evolution of an equal-mass massive black hole binary (MBHB).…

astro-ph.HE2024★ 2 cited

Fragments of harmony amid apparent chaos: a closer look at the X-ray quasi-periodic eruptions of the galaxy RX J1301.9+2747

Margherita Giustini, Giovanni Miniutti, Riccardo Arcodia +17

Quasi-periodic eruptions (QPEs) are an extreme X-ray variability phenomenon associated with low-mass supermassive black holes. First discovered in the nucleus of the galaxy GSN 069…

astro-ph.HE2024★ 28 cited

Ticking away: the long-term X-ray timing and spectral evolution of eRO-QPE2

R. Arcodia, I. Linial, G. Miniutti +11

Quasi-periodic eruptions (QPEs) are repeated X-ray flares from galactic nuclei. Despite some diversity in the recurrence and amplitude of eruptions, their striking regularity has m…

astro-ph.GA2024★ 2 cited

Partial alignment between jets and megamasers: Coherent versus selective accretion

Massimo Dotti, Riccardo Buscicchio, Francesco Bollati +3

Spins play a crucial role in the appearance, evolution, and occupation fraction of massive black holes (MBHs). To date, observational estimates of MBH spins are scarce, and the ass…

astro-ph.HE2024★ 2 cited

Testing EMRI models for Quasi-Periodic Eruptions with 3.5 years of monitoring eRO-QPE1

Joheen Chakraborty, Riccardo Arcodia, Erin Kara +13

Quasi-Periodic Eruptions (QPEs) are luminous X-ray outbursts recurring on hour timescales, observed from the nuclei of a growing handful of nearby low-mass galaxies. Their physical…

astro-ph.HE2024★ 27 cited

Electromagnetic signatures from accreting massive black hole binaries in time domain photometric surveys

Fabiola Cocchiararo, Alessia Franchini, Alessandro Lupi +1

We study spectral and time variability of accreting massive black hole binaries (MBHBs) at milli-pc separations surrounded by a geometrically thin circumbinary disc. We present the…

astro-ph.SR2024

The Santa Barbara Binary-Disk Code Comparison

Paul C. Duffell, Alexander J. Dittmann, Daniel J. D'Orazio +13

We have performed numerical calculations of a binary interacting with a gas disk, using eleven different numerical methods and a standard binary-disk setup. The goal of this study…

astro-ph.HE2024★ 13 cited

On the behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs

Alessia Franchini, Alessandra Prato, Cristiano Longarini +1

Using the 3D smoothed particle hydrodynamics code PHANTOM, we investigate the evolution of the orbital properties of massive black hole binaries embedded in massive discs where gra…

astro-ph.HE2024★ 22 cited

Emission signatures from sub-pc Post-Newtonian binaries embedded in circumbinary discs

Alessia Franchini, Matteo Bonetti, Alessandro Lupi +1

We study the dynamical evolution of quasi-circular equal mass massive black hole binaries embedded in circumbinary discs from separations of down to the merger,…

astro-ph.HE2023★ 8 cited

Neural Networks unveiling the properties of gravitational wave background from massive black hole binaries

Matteo Bonetti, Alessia Franchini, Bruno Giovanni Galuzzi +1

Massive black hole binaries (MBHBs) are binary systems formed by black holes with mass exceeding millions of solar masses, expected to form and evolve in the nuclei of galaxies. Th…

astro-ph.GA2023★ 1 cited

Massive Black Holes in Galactic Nuclei

David Izquierdo-Villalba, Alessandro Lupi, John Regan +2

Massive black holes are key inhabitants of the nuclei of galaxies. Moreover, their astrophysical relevance has gained significant traction in recent years, thanks especially to the…

astro-ph.HE2023

Comparing recent PTA results on the nanohertz stochastic gravitational wave background

The International Pulsar Timing Array Collaboration, G. Agazie, J. Antoniadis +242

The Australian, Chinese, European, Indian, and North American pulsar timing array (PTA) collaborations recently reported, at varying levels, evidence for the presence of a nanohert…

astro-ph.HE2023★ 320 cited

The second data release from the European Pulsar Timing Array I. The dataset and timing analysis

J. Antoniadis, S. Babak, A. -S. Bak Nielsen +66

Pulsar timing arrays offer a probe of the low-frequency gravitational wave spectrum (1 - 100 nanohertz), which is intimately connected to a number of markers that can uniquely trac…

astro-ph.HE2023★ 1k cited

The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

J. Antoniadis, P. Arumugam, S. Arumugam +95

We present the results of the search for an isotropic stochastic gravitational wave background (GWB) at nanohertz frequencies using the second data release of the European Pulsar T…