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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
verification ladder T0 review T1 audit T2 compute T3 formal

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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 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  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.

  2. Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields

    astro-ph.HE 2025-05 reject novelty 5.0 of 10

    The paper applies Schwinger pair production to toy magnetic field pulses in magnetically arrested disks and predicts detectable 1-3000 MHz synchrotron flux, but internal inconsistencies invalidate the claim.

  3. Road through Dark$\nu$ess: Probing dark matter-neutrino interactions using KM3-230213A

    hep-ph 2025-06 conditional novelty 4.0 of 10

    Using the 220 PeV event KM3-230213A, the authors set the highest-energy constraints to date on dark matter-neutrino scattering, and for energy-dependent cross sections they report some of the strongest existing limits.

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