Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 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.
citing papers explorer
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Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT
Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
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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.