Year: 2025
Type: article
Abstract: Although connections between flaring blazars and some IceCube neutrinos have been established, the dominant sources for the bulk extragalactic neutrino emissions are still unclear, and one widely suggested candidate is a population of radio galaxies. Because of their relatively low γ-ray radiation luminosities (Lγ), it is rather challenging to confirm such a hypothesis with the association between an incoming neutrino and a GeV γ-ray flare. Here, we report on the search for the GeV γ-ray counterpart of the neutrino IC-180213A and show that the nearby (z = 0.03) broad-line radio galaxy 3C 120 is the only known co-spatial GeV γ-ray source in a half-year epoch around the neutrino detection. An intense γ-ray flare, the second strongest one among the entire 16-year period, is temporally coincident with the detection of IC-180213A. Moreover, accompanying optical brightenings in the g band and V band are observed. We also find that the 3C 120, as a possible neutrino emitter, follows the Lγ-$ D_{L}^{2} $ correlation for the neutrino sources (candidates), including NGC 1068 and some blazars. These facts suggest that 3C 120 is a candidate for emitting high-energy neutrinos and may offer initial evidence of the radio galaxy origin of some PeV neutrinos.
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funders: National Aeronautics and Space Administration, Ohio State University, California Institute of Technology, National Natural Science Foundation of China, Jet Propulsion Laboratory, Goddard Space Flight Center, University of California, Los Angeles, Smithsonian Astrophysical Observatory, Russian Academy of Sciences, Planetary Science Division
Awards: G2881893134, G4025478747, G4503923430
OpenAlex ID: W7127195458
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