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From the 1 of 12 linked papers with an AI index.

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12 papers

gr-qc2026

All You Need is not : Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background

Haowen Zhong, Francesco Iacovelli, Vuk Mandic +1

Searches for the stochastic gravitational-wave background (SGWB) using ground-based detectors rely heavily on the cross-correlation estimator , whose statistical properti…

astro-ph.IM2026

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

Ulyana Dupletsa, Francesco Iacovelli, Mikhail Korobko +23

The paper evaluates how different design choices and noise characteristics of the Einstein Telescope affect its ability to detect and analyze various gravitational‑wave sources, us…

gr-qc2026

Improving low-latency multi-messenger follow-up of neutron star-black hole mergers with mode-by-mode filtering

Francesco Iacovelli, Digvijay Wadekar, Javier Roulet +2

Rapid parameter estimation for neutron star-black hole (NSBH) mergers is essential for deciding whether, where, and how electromagnetic facilities should follow up gravitational-wa…

gr-qc2026

The geometry of lunar gravitational wave detection

Jacopo Tissino, Filippo Santoliquido, Francesco Iacovelli +9

The Lunar Gravitational Wave Antenna (LGWA) is a planned gravitational wave detector on the Moon, targeting the deci-Hertz band and expected to deliver breakthrough discoveries acr…

gr-qc2026

Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123

Francesco Iacovelli, Jacopo Tissino, Jan Harms +1

We study the prospects of the Lunar Gravitational-Wave Antenna (LGWA), a proposed deci-Hz GW detector, to observe binary black holes (BBHs) and enable multiband science with ground…

gr-qc2026

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors

Francesco Iacovelli, Luca Reali, Emanuele Berti +3

Next-generation (XG) gravitational-wave detectors, such as Cosmic Explorer (CE) and the Einstein Telescope (ET), will observe compact binary coalescences at unprecedented rates and…