collaborators

8 papers

gr-qc2026

Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters

Luca Negri, Thomas C. K. Ng, Thibeau Wouters +13

The geometry of the Einstein Telescope, the proposed next-generation European gravitational-wave observatory, is yet to be finalized. Two competing designs are under consideration:…

gr-qc2026

Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession

Soumen Roy, Maria Haney, Geraint Pratten +2

When testing general relativity (GR) with gravitational wave observations, parametrized tests of deviations from the expected strong-field source dynamics are one of the most widel…

astro-ph.HE2025

Kilonova and progenitor properties of merger-driven gamma-ray bursts

P. Singh, G. Stratta, A. Rossi +6

Gamma-Ray Burst (GRB) prompt and afterglow emission, as well as a kilonova (KN), are the expected electromagnetic (EM) counterparts of Binary Neutron Star (BNS) and Neutron Star --…

gr-qc2025

Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise

Francesco Cireddu, Milan Wils, Isaac C. F. Wong +3

The Einstein Telescope faces a critical data analysis challenge with correlated noise, often overlooked in current parameter estimation analyses. We address this issue by presentin…

gr-qc2025

Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements

Harsh Narola, Thibeau Wouters, Luca Negri +10

Gravitational Wave (GW) detectors routinely encounter transient noise bursts, known as glitches, which are caused by either instrumental or environmental factors. Due to their high…

astro-ph.HE2025

Inferring neutron star merger ejecta morphologies with kilonovae

Brendan L. King, Soumi De, Oleg Korobkin +2

In this study we incorporate a new grid of kilonova simulations produced by the Monte Carlo radiative transfer code SuperNu in an inference pipeline for astrophysical transients, a…