A neutrino flare in GB6 J1542+6129 precedes gamma-ray and radio activity by about one year, indicating upstream neutrino production near the AGN central engine.
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2026 2representative citing papers
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.
citing papers explorer
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Upstream neutrino production and delayed jet emission in the blazar GB6 J1542+6129
A neutrino flare in GB6 J1542+6129 precedes gamma-ray and radio activity by about one year, indicating upstream neutrino production near the AGN central engine.
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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.