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Leveraging Artificial intelligence for Astrophysical Source parameter Estimation and Rapid electromagnetic follow-up with the future space-based Gravitational Waves Observatory

CORDIS · observation · Publication date unknown

Leveraging Artificial intelligence for Astrophysical Source parameter Estimation and Rapid electromagnetic follow-up with the future space-based Gravitational Waves Observatory The Laser Interferometer Space Antenna (LISA), a milli-Hertz gravitational wave (GW) observatory, has extraordinary scientific potential. It is expected to revolutionize multimessenger astrophysics in the mid-2030s through synergies between LISA and both space- and Earth-based electromagnetic (EM) observatories. Mergers of supermassive black hole binary systems will be primary sources for these multimessenger studies. LISA will detect GWs emitted during the pre-merger phase and pinpoint the source location, allowing EM observatories with narrow fields of view to search for potential counterparts. For this synergy to be effective, rapid alerts of sky positions and coalescence timing are crucial—not only at the moment of merge

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award

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SIGNED

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EU

value

416941.44

unit

EUR