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From the 1 of 35 linked papers with an AI index.

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35 papers

astro-ph.CO2026

GUEST: Gravitational Universe Exploration with Satellite Tracking. A passive satellite laser-ranging mission for the dark gravitational Universe

Diego Blas, Aurélien Hees, F. Javier Atapuerca +78

GUEST is a space mission concept whose central objective is the detection of gravitational waves (GWs) in the microhertz band -- a physics-rich frequency window that no other prese…

astro-ph.HE2026

Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources

Alice Perego, Matteo Bonetti, Alberto Sesana +2

The paper evaluates the detection capabilities of three proposed post‑LISA space‑based gravitational‑wave missions (μAres, AMIGO, and the Decihertz Observatory) by modeling astroph…

astro-ph.GA2026

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

Stephanie Buttigieg, Debora Sijacki, Christopher J. Moore +2

The recent detection of a gravitational wave background (GWB) by pulsar timing arrays (PTAs) may represent the first evidence of gravitational waves from merging supermassive black…

astro-ph.IM2026

LISA and the LISA Science Team

Anna Heffernan, Chiara Caprini, Neil Cornish +19

LISA, the Laser Interferometer Space Antenna, due to launch mid-2035, is a large class space mission by the European Space Agency (ESA). In partnership with NASA and ESA-member sta…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…

astro-ph.HE2026

Archival Multiband Gravitational-Wave Signals from Massive Black Hole Binary Mergers

Alexander W. Criswell, Stephen R. Taylor, Kris Pardo +4

While massive black hole binaries (MBHBs) merge at gravitational-wave frequencies above the pulsar timing array (PTA) sensitivity band, we show that they leave orphaned low-frequen…