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Improving the Sensitivity of Gravitational Wave Detection with Weighted Conformal Prediction

arxiv.org/abs/2609.11401

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Updated 4 h ago · first seen 11 Sept 2026

paper_01M294FQYFK6MF40DF058XAJ8N

Published
11 Sept 2026
T1 · 4 h ago
arXiv
2609.11401
T1 · 4 h ago
Category
gr-qc
T1 · 4 h ago

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Claim history for Abstract
ValueValid from → toStatusSourceConfidenceExtractor
In the last decade, kilometre-scale interferometric gravitational-wave detectors have observed hundreds of compact binary mergers, the majority of which are binary black holes. However, the data are noise-dominated, and multiple independent search algorithms (pipelines) are used to enhance sensitivity and improve robustness. Rather than the standard approach of selecting the most significant pipeline output, we combine the outputs from all pipelines using a conformal prediction-based framework to provide statistically rigorous confidence estimates for candidate events. While combining pipelines improves sensitivity and ranking robustness, it requires a principled statistical framework that remains valid as data properties evolve across observing runs. A key challenge is distribution shifts between simulated datasets used for training and calibration and the real, unlabelled, observations used for testing, which can invalidate coverage guarantees and bias confidence estimates. In this work, we address this challenge by incorporating likelihood-ratio reweighting into our conformal prediction framework to account for covariate shift. Using mock datasets containing simulated signals, we demonstrate that weighted conformal prediction restores well-calibrated coverage under covariate shift and increases the confidence of events near the detection threshold, recovering true signals that would otherwise be missed.currentcurrentarXiv (Atom API + RSS)T1highdeterministic

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