collaborators

5 papers

astro-ph.HE2026

Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays

Sara Manzini, Stanislav Babak

Pulsar timing array (PTA) experiments are searching for gravitational waves (GWs) in the nanohertz band. The primary GW sources targeted by PTAs include populations of inspiralling…

astro-ph.GA2026

The multimessenger view of Pulsar Timing Array black holes with the Horizon-AGN simulation

Hippolyte Quelquejay Leclere, Kunyang Li, Marta Volonteri +5

We use the Horizon-AGN cosmological simulation to study the properties of supermassive black hole binaries (MBHBs) contributing most to the gravitational wave background (GWB) sign…

gr-qc2025

Effective-one-body modelling of eccentric supermassive black hole binaries for Pulsar Timing Array

Sara Manzini, Stanislav Babak

Pulsar Timing Arrays (PTAs) observations will detect gravitational waves (GWs) from the early inspiral phase of supermassive black hole binaries (SMBHBs) with orbital periods of we…

gr-qc2025

Contamination of transient gravitational waves in LISA data by gaps and glitches

Jonathan R. Gair, Senwen Deng, Stanislav Babak

We present a probabilistic framework to quantify the impact of artefacts (glitches and gaps) in LISA data on transient gravitational wave signals. By modeling both artefacts and tr…

gr-qc2025

Fast detection and reconstruction of merging Massive Black Hole Binary signals

Senwen Deng, Stanislav Babak, Sylvain Marsat

The Laser Interferometer Space Antenna (LISA) will detect gravitational waves from the population of merging massive black holes binaries (MBHBs) throughout the Universe. The LISA…