27–30 Jan 2026
Soeterbeeck Conference Centre,
Europe/Amsterdam timezone

Session

Session 1

27 Jan 2026, 16:00
Tuinzaal (Soeterbeeck Conference Centre,)

Tuinzaal

Soeterbeeck Conference Centre,

Elleboogstraat 2 5352LP Deursen-Dennenburg, The Netherlands

Conveners

Session 1: Jet Physics in AGN

  • Aylecia Lattimer (Anton Pannekoek Institute, University of Amsterdam)

Description

Presentations & QA

Presentation materials

There are no materials yet.

  1. Ruby Duncan (University of Amsterdam)
    27/01/2026, 16:00
    Presentation

    My work involves developing and applying a physically motivated multi-zone jet model to a variety of low luminosity active galactic nuclei, fitting their radio to X-ray spectral energy distributions to constrain and better understand micro/macro jet physics and particle acceleration, and how it might vary between sources. Building on this, a new analysis pipeline is being developed that...

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  2. RITTICK ROY (UNIVERSITY OF AMSTERDAM)
    27/01/2026, 16:21
    Presentation

    A key open question in astrophysics is how particles are heated and accelerated in accretion flows and how this shapes observed emission. We present a new method for reconstructing the connection between plasma dynamics and particle acceleration in the accretion flow of the LLAGN M87*, using the 2017 Event Horizon Telescope multi-wavelength campaign as a prototype. Our Bayesian framework...

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  3. Marc Klinger-Plaisier (Anton Pannekoek Institute - University of Amsterdam)
    27/01/2026, 16:42
    Presentation

    The super-fast (~day), very-high-energy (VHE; >0.1 TeV) photon flares from the nearby active galactic nucleus M87 provide a unique, exciting opportunity to fast-forward our understanding of particle acceleration in jets. Despite 5 detected VHE flares in the last 20 years and extensive multiwavelength (MWL) campaigns, the process and location of these VHE flares in the jet are still not fully...

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  4. Subhrat Praharaj (University of Amsterdam)
    27/01/2026, 17:03
    Presentation

    We investigate the composition and dynamics of black hole accretion jets using novel high-res GRMHD simulations. By deploying Lagrangian composition tracers and adaptive mesh refinement (AMR), we achieve two goals: 1) We precisely track how disk material mixes into the jet and how jet plasma entrains into the surrounding sheath, and 2) We maintain high resolution dynamically within the jet and...

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  5. Michael Florian Wondrak
    27/01/2026, 17:24
    Presentation

    I will review several energy extraction mechanisms (classical and quantum) to facilitate discussions on approaching the Blandford-Znajek process in the future.

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  6. 27/01/2026, 17:45
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