From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts
Andrea Caputo, Valerie Domcke
astro-ph.GA, astro-ph.CO, astro-ph.HE, gr-qc
Submitted: 2026-07-28
Comments: 22 pages, 10 figures; Claude Code-generated repository reproducing all results at https://github.com/andrea0292/s2-to-lisa
Code: https://github.com/andrea0292/s2-to-lisa
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Prospects for observing extreme-mass-ratio inspirals with LISA
- Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
- Gravitational wave background from extreme mass ratio inspirals
- Gravitational wave energy spectrum of a parabolic encounter
- Observing the Galaxy's massive black hole with gravitational wave bursts
- Gravitational Wave Peep Contributions to Background Signal Confusion Noise for LISA
- Extreme-mass-ratio-bursts from extragalactic sources
- Expectations for extreme-mass-ratio bursts from the Galactic Centre
- Steady state relativistic stellar dynamics around a massive black hole
- Relativistic Dynamics and Extreme Mass Ratio Inspirals
- Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei
- Dynamics around supermassive black holes: Extreme mass-ratio inspirals as gravitational-wave sources
- Semi-Analytical Fokker Planck Models for Nuclear Star Clusters
- Strong mass segregation around a massive black hole
- Multi-wavelength constraints on the local black hole occupation fraction
- Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits
- LISA Definition Study Report
- The Galactic Center Massive Black Hole and Nuclear Star Cluster
- First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
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