[astro-ph.IM] Building on prior FAST targeted and blind SETI campaigns toward 33 exoplanet systems, we introduce a wavelet-integrated search pipeline for narrowband technosignature candidates in radio dynamic spectra.
At its core, the pipeline uses a Multi-Scale Wavelet Net (MSWNet) to produce an interpretable multi-resolution representation, followed by a lightweight parameter estimator for endpoint localization.
Rather than relying solely on hard-threshold drift searches, the pipeline reframes narrowband detection as wavelet-guided feature extraction followed by endpoint regression, morphology-aware filtering, raw-data S/N validation, and multi-beam anticoincidence veto. Applied to real FAST data, the pipeline recovers representative events from prior analyses and produces a compact set of veto-ready candidates for downstream inspection.
The resulting workflow preserves interpretability, low regression complexity, and auditable threshold control, making it readily transferable to other radio surveys and large-scale technosignature searches.
Zi-Qi Li, Jian-Kang Li, Zhe-Wei Luo, Chen-Xu Guan, Yu-Tong Fan, Zhen-Zhao Tao, Xiao-Hang Luan, Bo-Lun Huang, Yu Hu, Peng-Yu Li, Pu-Fan Liu, Kang Jiao, Tong-Jie Zhang, Hai-Yan Zhang, Peng Jiang, Rui Li, Liang Gao
Comments: 19 pages, 10 figures. Resubmitted to AJ after revisions
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2605.23739 [astro-ph.IM] (or arXiv:2605.23739v2 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2605.23739
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Submission history
From: Zi-Qi Li
[v1] Fri, 22 May 2026 15:13:59 UTC (25,463 KB)
[v2] Tue, 7 Jul 2026 17:32:40 UTC (25,462 KB)
https://arxiv.org/abs/2605.23739
Astrobiology, SETI,
