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Relativistic Jets of Blazars

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arxiv 2003.06322 v2 pith:47RWAEBP submitted 2020-03-13 astro-ph.HE

Talvikki Hovatta , Elina Lindfors This is my paper · ORCID
classification astro-ph.HE
keywords jetsblazarsrelativisticcoverobservationsactivebeenclose
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Relativistic jets of active galactic nuclei have been known to exist for 100 years. Blazars with their jet pointing close to our line of sight are some of the most variable and extreme objects in the universe, showing emission from radio to very-high-energy gamma rays. In this review, we cover relativistic jets of blazars from an observational perspective with the main goal of discussing how observations can be used to constrain theoretical models. We cover a range of topics from multiwavelength observations to imaging of jets with a special emphasis on current open questions in the field.

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Cited by 1 Pith paper

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  1. Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    Using neural-posterior-estimation simulation-based inference on the MOJAVE FSRQ sample, the authors infer a Lorentz factor distribution slope b = -1.32 (+0.20, -0.19), consistent with X-ray binary jets at 2 sigma.

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