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Systematic study reveals SNR requirements for chirp tracking in gravitational wave datasets, suggesting improved methods.
Consolidates Papers 7–10 of the Neural Lagrangian Series. Four methods applied to GW150914, GW151226, GW170817. Derives per-window SNR requirement (SNR_opt ≥ 40) for template-free chirp tracking. GW150914 whitened spectrogram ridge recovers f ∈ [30,83] Hz within 11% of GR prediction. BBH/BNS effective coefficient ratio 2.22×. Proposes hybrid matched-filter + PySR pipeline for Einstein Telescope data
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Muhammad Hanif (2026) studied this question.
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