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PKS 1424+240: yet another masquerading BL Lac object as a possible IceCube neutrino source

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arxiv 2202.04363 v1 pith:24J2Z4UW submitted 2022-02-09 astro-ph.HE astro-ph.GAhep-exhep-ph

PKS 1424+240: yet another masquerading BL Lac object as a possible IceCube neutrino source

classification astro-ph.HE astro-ph.GAhep-exhep-ph
keywords neutrinosourcesicecubeblazarhighmasqueradingobjectother
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We show that the blazar PKS 1424+240, which has been recently associated by IceCube with a neutrino excess at the $3.3\,\sigma$ level together with three other sources, is similar to the first plausible non-stellar neutrino source, TXS 0506+056, in being also a masquerading BL Lac object, i.e., intrinsically a flat-spectrum radio quasar with hidden broad lines and a standard accretion disk. We point out that these two sources share other properties, including spectral energy distribution, high powers, parsec scale properties, and possibly radio morphology. We speculate that the relatively rare combination of proton-loaded jets, possibly typical of high-excitation sources, and efficient particle acceleration processes, related to their relatively high synchrotron peak frequencies, might favour neutrino production in these two sources. GB6 J1542+6129, which has also recently appeared twice in a list of IceCube associations, seems also to belong to this rare blazar sub-class, which includes at most ~ 20 Fermi-4LAC blazars.

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Forward citations

Cited by 3 Pith papers

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  2. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 accept novelty 2.5

    AGN (jetted and non-jetted) are viable high-energy neutrino sources, with TXS 0506+056 and NGC 1068 as the only statistically significant associations so far, while gamma-ray blazars contribute only a small fraction o...

  3. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 unverdicted novelty 2.0

    Review summarizing correlations between astrophysical neutrinos and gamma-ray/radio AGN, specific source associations, proposed production mechanisms, and future prospects.