Inpainting to search for premerger massive black hole binaries in realistic LISA datasets

arXiv:2605.13738 · astro-ph.IM, astro-ph.CO, gr-qc, hep-ex · Submitted 2026-05-13 · Read on arXiv

astro-ph.IM, astro-ph.CO, gr-qc, hep-ex

Submitted: 2026-05-13

Updated: 2026-10-09

Terminology

• Signal-to-Noise Ratio — 28× in this paper
• Signal-to-Noise Ratio (SNR) — 3× in this paper · explained in 3 episodes
• Large Interferometer Space Antenna — 2× in this paper
• Accuracy — 1× in this paper · explained in 1 episode

Sources

• Laser Interferometer Space Antenna
• LISA Definition Study Report
• Astrophysics with the Laser Interferometer Space Antenna
• The Mock LISA Data Challenges: An overview
• A How-To for the Mock LISA Data Challenges
• Report on the first round of the Mock LISA Data Challenges
• Report on the second Mock LISA Data Challenge
• The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
• An overview of the second round of the Mock LISA Data Challenges
• The Mock LISA Data Challenges: from Challenge 3 to Challenge 4
• The LISA Data Challenges
• Premerger observation and characterization of massive black hole binaries
• Detection and Prediction of Future Massive Black Hole Mergers with Machine Learning and Truncated Waveforms
• Premerger detection of massive black hole binaries using deep learning
• Pre-Merger Localization of Gravitational-Wave Standard Sirens With LISA: Triggered Search for an Electromagnetic Counterpart
• Sky localization of complete inspiral-merger-ringdown signals for nonspinning massive black hole binaries
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Detectability of modulated X-rays from LISA's supermassive black hole mergers
• Extraction of gravitational wave signals from LISA data in the presence of artifacts
• Detecting Gravitational Waves in Data with Non-Gaussian Noise

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