activity
20152023
most citedGW190521 as a merger of Proca stars: a potential new vector boson of eV

230 citations · 802 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2023★ 2 cited

Bayesian inference from gravitational waves in fast-rotating, core-collapse supernovae

Carlos Pastor-Marcos, Pablo Cerdá-Durán, Daniel Walker +4

Core-collapse supernovae (CCSNe) are prime candidates for gravitational-wave detectors. The analysis of their complex waveforms can potentially provide information on the physical…

gr-qc2023★ 4 cited

Comparison of neural network architectures for feature extraction from binary black hole merger waveforms

Osvaldo Gramaxo Freitas, Juan Calderón Bustillo, José A. Font +3

We evaluate several neural-network architectures, both convolutional and recurrent, for gravitational-wave time-series feature extraction by performing point parameter estimation o…

physics.comp-ph2023★ 4 cited

Gradient-Annihilated PINNs for Solving Riemann Problems: Application to Relativistic Hydrodynamics

Antonio Ferrer-Sánchez, José D. Martín-Guerrero, Roberto Ruiz de Austri +2

We present a novel methodology based on Physics-Informed Neural Networks (PINNs) for solving systems of partial differential equations admitting discontinuous solutions. Our method…

astro-ph.HE2023★ 12 cited

Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability

Marco Drago, Haakon Andresen, Irene Di Palma +2

The gravitational wave (GW) and neutrino signals from core-collapse supernovae (CCSNe) are expected to carry pronounced imprints of the standing accretion shock instability (SASI).…

gr-qc2022★ 18 cited

Virgo Detector Characterization and Data Quality: tools

F. Acernese, M. Agathos, A. Ain +491

Detector characterization and data quality studies -- collectively referred to as {\em DetChar} activities in this article -- are paramount to the scientific exploitation of the jo…

gr-qc2022★ 60 cited

Virgo Detector Characterization and Data Quality: results from the O3 run

F. Acernese, M. Agathos, A. Ain +491

The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave (GW) signals in the past few years, alongside the two Adv…

gr-qc2022★ 44 cited

Impact of the wave-like nature of Proca stars on their gravitational-wave emission

Nicolas Sanchis-Gual, Juan Calderón Bustillo, Carlos Herdeiro +4

We present a systematic study of the dynamics and gravitational-wave emission of head-on collisions of spinning vector boson stars, known as Proca stars. To this aim we build a cat…

gr-qc2022★ 7 cited

Virgo Detector Characterization and Data Quality during the O3 run

F. Acernese, M. Agathos, A. Ain +491

The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave signals in the past few years, alongside the two LIGO ins…

gr-qc2022★ 22 cited

The Virgo O3 run and the impact of the environment

F. Acernese, M. Agathos, A. Ain +486

Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient…

gr-qc2021★ 20 cited

Classification of the core-collapse supernova explosion mechanism with learned dictionaries

Ainara Saiz-Pérez, Alejandro Torres-Forné, José A. Font

Core-collapse supernovae (CCSN) are a prime source of gravitational waves. Estimations of their typical frequencies make them perfect targets for the current network of advanced, g…

gr-qc2020★ 71 cited

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369

Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…

gr-qc2020★ 230 cited

GW190521 as a merger of Proca stars: a potential new vector boson of eV

Juan Calderón Bustillo, Nicolas Sanchis-Gual, Alejandro Torres-Forné +6

Advanced LIGO-Virgo reported a short gravitational-wave signal (GW190521) interpreted as a quasi-circular merger of black holes, one populating the pair-instability supernova gap,…

astro-ph.HE2018★ 95 cited

Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - II. Spacetime perturbations

Alejandro Torres-Forné, Pablo Cerdá-Durán, Andrea Passamonti +2

Improvements in ground-based, advanced gravitational wave (GW) detectors may allow in the near future to observe the GW signal of a nearby core-collapse supernova. For the most com…

astro-ph.SR2018★ 27 cited

Total-variation methods for gravitational-wave denoising: performance tests on Advanced LIGO data

Alejandro Torres-Forné, Elena Cuoco, Antonio Marquina +2

We assess total-variation methods to denoise gravitational-wave signals in real noise conditions, by injecting numerical-relativity waveforms from core-collapse supernovae and bina…

astro-ph.SR2017★ 89 cited

Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - I. Cowling approximation

Alejandro Torres-Forné, Pablo Cerdá-Durán, Andrea Passamonti +1

Gravitational waves from core-collapse supernovae are produced by the excitation of different oscillation modes in the proto-neutron star (PNS) and its surroundings, including the…

astro-ph.IM2016★ 52 cited

Denoising of gravitational wave signals via dictionary learning algorithms

Alejandro Torres-Forné, Antonio Marquina, José A. Font +1

Gravitational wave astronomy has become a reality after the historical detections accomplished during the first observing run of the two advanced LIGO detectors. In the following y…

astro-ph.IM2016★ 1 cited

Denoising of gravitational-wave signal GW150914 via total-variation methods

Alejandro Torres-Forné, Antonio Marquina, José A. Font +1

We apply a regularized Rudin-Osher-Fatemi total variation (TV) method to denoise the transient gravitational wave signal GW150914. We have previously applied TV techniques to denoi…

astro-ph.SR2015★ 44 cited

Are pulsars born with a hidden magnetic field?

Alejandro Torres-Forné, Pablo Cerdá-Durán, José A. Pons +1

The observation of several neutron stars in the center of supernova remnants and with significantly lower values of the dipolar magnetic field than the average radio-pulsar populat…