Publications

We study the impact of the baseline on the localization of BBHs observed by Cosmic Explorer.

We present an exhaustive discussion of the scientific propsects of ET.

We extend our previous analysis of systematics in LISA, including aligned spins and more massive systems.

Summary of the talks and discussions from the workshop deci-Hz Gravitational Wave Observations on the Moon and Beyond.

We assess the impact of an insufficient higher-order mode content in waveform templates on the parameter estimation of LISA massive BH binary systems.

We investigate the prospects of observing different electromagnetic emissions associated to binary neutron star and black hole-neutron star mergers detected through gravitational waves at ET and CE.

We study the prospects of observing binary black holes with the Lunar Gravitational-Wave Antenna.

We examine the scientific potential of different ET designs in combination with CE.

We study how to speed-up sampling in GW parameter estimation.

We study how environmental effects can affect PE at ET and LISA.

We develop a Fisher tool for forecasts on population analyses at third-generation detectors.

We provide a first comprehensive analysis of the Lunar Gravitational-wave Antenna science case including its multi-messenger aspects and lunar science.

We develop a way to perform unbiased estimations of the expansion rate of the Universe from gravitational-wave + γ-ray burst detections and a new gravitational-wave likelihood approximant.

We compute the impact of astrophysical “confusion noise” in the search for cosmological gravitational-wave backgrounds.

We derive the spectral density of the stochastic gravitational-wave background generated by compact binary coalescences.

We examine the scientific potential of a European third-generation network comprising two L-shaped detectors, one underground and one on-surface.

We study the prospects of classifying binary black holes originating from Population III stars observed through gravitational waves at the Einstein Telescope using machine learning.

We investigate the prospects of observing electromagnetic counterparts to black hole-neutron star mergers detected through gravitational waves during O4 and O5.

We develop a code to perform a joint population and cosmological inference on gravitational-wave data and galaxy catalogs, and apply it to simulated O4 and O5 catalogs of gravitational waves.

We study how binary neutron star mergers observations at the Einstein Telescope can improve our understanding of their equation of state.

We analyze in detail the impact of different designs for the Einstein Telescope on our future capability of observing key quantities characterizing primordial black hole mergers and also perform a population analysis.

We examine the scientific perspectives of different designs for the Einstein Telescope, with a detailed evaluation of the science case.

We provide useful metrics to assess the capabilities of third-generation gravitational-wave detectors in the observation of high-redshift sources.

Prospects of combining γ-ray burst polarization measurements and gravitational-wave observations to extract information on the γ-ray bursts emission model.

Up-to-date forecasts of the capabilities of Einstein Telescope and Cosmic Explorer to observe compact binary mergers.

We release, review, and validate the GWFAST code!

We show how the narrowness of the binary neutron star mass distribution can give clear signatures of modified gravity.

We show how quadruply lensed gravitational-wave events can be an extremely valuable candidate to constrain modifications of GR at cosmological scales.

We exploit gravitational-wave detections and a galaxy catalog to obtain constraints on the expansion rate of the Universe and possible deviations from GR at cosmological scales. A public code is also released!