Giulia Capurri
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View article: The Science of the Einstein Telescope
The Science of the Einstein Telescope Open
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 objectives, providing state-of-the-art predictions for the ca…
View article: Enhancing the localization of gravitational-wave hosts with SKYFAST: Rapid volume and inclination angle reconstruction
Enhancing the localization of gravitational-wave hosts with SKYFAST: Rapid volume and inclination angle reconstruction Open
Context. The scientific impact of GW170817 strongly supports the suggestion that we need an efficient electromagnetic follow-up campaign for gravitational-wave event candidates. The success of these campaigns critically depends on a fast a…
View article: Impact of correlated noise on the reconstruction of the stochastic gravitational wave background with Einstein Telescope
Impact of correlated noise on the reconstruction of the stochastic gravitational wave background with Einstein Telescope Open
Einstein Telescope (ET) is a proposed next-generation Gravitational Wave (GW) interferometer designed to detect a large number of astrophysical and cosmological sources with unprecedented sensitivity. A key target for ET is the detection o…
View article: Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction Open
The scientific impact of GW170817 strongly supports the need for an efficient electromagnetic follow-up campaign to gravitational-wave event candidates. The success of such campaigns depends critically on a fast and accurate localization o…
View article: Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background Open
The stochastic gravitational-wave background (SGWB) produced by merging neutron stars exhibits a peak in the kHz band. In this paper, we develop a theoretical framework to exploit this distinctive feature through a Markov Chain Monte Carlo…
View article: Searching for Anisotropic Stochastic Gravitational-wave Backgrounds with Constellations of Space-based Interferometers
Searching for Anisotropic Stochastic Gravitational-wave Backgrounds with Constellations of Space-based Interferometers Open
Many recent works have shown that the angular resolution of ground-based detectors is too poor to characterize the anisotropies of the stochastic gravitational-wave background (SGWB). For this reason, we asked ourselves if a constellation …
View article: Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers Open
Many recent works have shown that the angular resolution of ground-based detectors is too poor to characterize the anisotropies of the stochastic gravitational-wave background (SGWB). For this reason, we asked ourselves if a constellation …
View article: Detectability of the Cross-Correlation between CMB Lensing and Stochastic GW Background from Compact Object Mergers
Detectability of the Cross-Correlation between CMB Lensing and Stochastic GW Background from Compact Object Mergers Open
The anisotropies of the Stochastic Gravitational-Wave Background (SGWB), produced by merging compact binaries, constitute a possible new probe of the Large-Scale Structure (LSS). However, the significant shot noise contribution caused by t…
View article: Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers Open
The anisotropies of the Stochastic Gravitational-Wave Background (SGWB) produced by merging compact binaries constitute a possible new probe of the Large-Scale Structure (LSS). However, the significant shot noise contribution caused by the…
View article: Intensity and anisotropies of the stochastic gravitational wave background from merging compact binaries in galaxies
Intensity and anisotropies of the stochastic gravitational wave background from merging compact binaries in galaxies Open
We investigate the isotropic and anisotropic components of the Stochastic Gravitational Wave Background (SGWB) originated from unresolved merging compact binaries in galaxies. We base our analysis on an empirical approach to galactic astro…
View article: Letter-to-the Editor: Focal cerebral arteriopathy and acute ischaemic stroke in children: A diagnostic-therapeutical conundrum
Letter-to-the Editor: Focal cerebral arteriopathy and acute ischaemic stroke in children: A diagnostic-therapeutical conundrum Open