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arXiv · 2405.10684

Changing Look of the optical spectrum of the MeV Blazar PKS 0446+112 (4FGL J0449.1+1121)

Simona Paiano·Renato Falomo·Aldo Treves·Riccardo Scarpa·Boris Sbarufatti
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Abstract

Following the high activity of the gamma-ray Fermi source 4FGL J0449.1+1121 (PKS 0446+112), possibly associated with a IceCube neutrino event IC-240105A, we obtained optical spectroscopy with the Gran Telescopio Canarias of the counterpart. We detect a clear emission line at 3830 Ang identified as Ly$\alpha$ that confirms the redshift of source at z=2.153. Comparing with previous spectroscopy, we find an increase of the continuum by a factor $\sim$10, and a significant decrease of the CIV 1550 emission line flux by a factor $\sim$5. This produces a dramatic drop of the Equivalent Width from $\sim$20 Ang to 0.8 Ang, which is suggestive of a very high jet activity. The Full Width Half Maximum of the emission lines are midway (1000 - 2000 km/s) between those typical of the broad and narrow regions of quasars. Based on this, the source classification is intermediate between Flat Spectrum Radio Quasar and BL Lac object.

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Simona Paiano, Renato Falomo, Aldo Treves, Riccardo Scarpa, Boris Sbarufatti. 2024-05-17. Changing Look of the optical spectrum of the MeV Blazar PKS 0446+112 (4FGL J0449.1+1121). https://arxiv.org/abs/2405.10684

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