Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.
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2025 2representative citing papers
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.
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Association of the IceCube neutrinos with CAZ blazar light curves
Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.
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The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.