Accurate standard siren cosmology with joint gravitational-wave and γ-ray burst observations
We develop a way to perform unbiased estimations of the expansion rate of the Universe from GW+GRB detections and a new GW likelihood approximant
Here you can find a complete list of my publications. Clicking on any of the links below will redirect you to the abstract and details of my contributions to the papers I am not the first author of. A PDF version of my publication list can be downloaded clicking the button below
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We develop a way to perform unbiased estimations of the expansion rate of the Universe from GW+GRB detections and a new GW likelihood approximant
We study the prospects of classifying BBH originating from Population III stars observed through GWs at ET using machine learning
We provide a first comprehensive analysis of the LGWA science case including its multi-messenger aspects and lunar science
We develop a code to perform a joint population and cosmological inference on GW data and galaxy catalogs, and apply it to simulated O4 and O5 catalogs of GW
We investigate the prospects of observing electromagnetic counterparts to black hole-neutron star mergers detected through gravitational waves during O4 and O5
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!