First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.
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4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4verdicts
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Derives B*(d) and N*(d) for AGN jet cores from self-absorbed synchrotron emission model with power-law assumptions on Doppler factor, Lorentz factor, B, and N versus jet width d.
New VERITAS observations of the 2017 VHE flare from NGC 1275, with multiwavelength SEDs, support a two-component blob-in-jet model placing gamma-ray emission near the C3 radio component at a 10-degree viewing angle.
SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
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VLTI-GRAVITY observations of blazars
First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.