Methods for Detecting Gravitational Waves from mini-Extreme-Mass-Ratio Inspirals I: Statistics Based on Time-Frequency Signal TracksDec 1, 2025·Zi-Xuan Wang,Gong Cheng,Ju Chen,Huai-Ke GuoAndrew L. Miller· 0 min read PDF CiteLast updated on Dec 1, 2025 AuthorsAndrew L. MillerAssociate Professor ← BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform Dec 1, 2025Methods for Detecting Gravitational Waves from mini-Extreme-Mass-Ratio Inspirals II: A Spectral-Leakage-Aware Framework Dec 1, 2025 →