Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
2019 2verdicts
UNVERDICTED 2representative citing papers
PKS 0346-27 displayed a prolonged 2018 gamma-ray high state with ~1.5-hour variability, harder spectrum, and SED transition from LSP to ISP class, with one-zone leptonic modeling indicating lower magnetic field, larger radius, and higher electron energies than in quiescence.
citing papers explorer
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Gamma-ray emission in radio galaxies under the VLBI scope -- I. Parsec-scale kinematics and high-energy properties of $\gamma$-ray detected TANAMI radio galaxies
Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.
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The large gamma-ray flare of the FSRQ PKS 0346-27
PKS 0346-27 displayed a prolonged 2018 gamma-ray high state with ~1.5-hour variability, harder spectrum, and SED transition from LSP to ISP class, with one-zone leptonic modeling indicating lower magnetic field, larger radius, and higher electron energies than in quiescence.