collaborators

6 papers

gr-qc2026

The impact of physically motivated calibration errors on search pipeline detection parameters for broadband burst Signals

Milan Wils, Brad Ratto, Jeffrey S. Kissel +4

Imperfections in the calibration of gravitational wave observatories introduce frequency dependent amplitude and phase errors on the measured GW signal. Previous unmodelled burst s…

gr-qc2025

Bayesian Calibration of Gravitational-Wave Detectors Using Null Streams Without Waveform Assumptions

Isaac C. F. Wong, Francesco Cireddu, Milan Wils +4

We introduce a Bayesian null-stream method to constrain calibration errors in closed-geometry gravitational-wave (GW) detector networks. Unlike prior methods requiring electromagne…

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

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

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…

gr-qc2025

Potential impact of noise correlation in next-generation gravitational wave detectors

Isaac C. F. Wong, Peter T. H. Pang, Milan Wils +3

Building upon the statistical formulation for parameter estimation (PE) in the presence of correlated noise proposed by Cireddu et al., we present the initial study to incorporate…