Table of Contents

Extragalactic jets from radio to gamma-rays Eileen T. Meyer; Multiwavelength monitoring of the nucleus in PBC J2333.9-2343: a giant radio galaxy with a blazar-like core Lorena Hernandez-Garcia; A WISE perspective of the blazar hunt in the γ-ray sky Francesco Massaro; Gamma-ray flux distribution analysis on 145 gamma-ray bright blazars Maria Petropoulou; Milliarcsecond core size dependence of the radio variability of blazars Po-Chih Hsu; Understanding the interplay between jets and ISM for winged radio galaxies Gourab Giri; Exploring connections between the VLBI and optical morphology of AGNs and their host galaxies David Fernández; RAD@home discovery of a one-sided radio jet hitting the companion galaxy_x000D_ Ananda Hota; RAD@home RGB-maker web-tool for citizen science research in multi-wavelength study of AGNs with radio jets Avinash Kumar; RAD@home Inter-University Collaboratory for citizen science in galaxy evolution with multi wavelength RGB images Megha Rajoria; 3D PIC simulations for relativistic jets with a toroidal magnetic field Kenichi Nishikawa; Effect of inverse Compton cooling on relativistic particles accelerated at shear boundary layers in relativistic jets Tej Chand; Particle acceleration via magnetic reconnection in large-scale MHD jet simulations Anna Lisa Celotti; Radio polarization: A powerful resource for understanding the blazar divide Janhavi Baghel; The microvariability and wavelength dependence of polarization vector of BL Lacertae in the outburst 2020 to 2021 Ryo Imazawa; Intraday variations of polarization vector in blazars: a key to the optical jet structure? Elena Shablovinskaya; Identifying γ-ray emitting blazars in the PASIPHAE era Nikos Mandarakas; Scientific potential of MeV polarimetry for relativistic jets Haocheng Zhang; J2102+6015: A potential high-redshift multimessenger Leonid Gurvits; VLBI scrutiny of a new neutrino-blazar multiwavelength-flare coincidence Florian Eppel; Redshift determination of blazars for the Cherenkov Telescope Array Eli Kasai

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Blazar experts provide answers to long-standing questions about how these powerful relativistic jets form and how they shine.