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FRANCI 2025

28 July 2025
Stephanshof Bamberg
Europe/Berlin timezone

Contribution List

17 out of 17 displayed
  1. 1. Welcome
    Max & Lea
    28/07/2025, 10:00
  2. 2. Hydrodynamic Simulations of the Supernova Remnant Puppis A with PLUTO
    Marie Prucker (Remeis Observatory)
    28/07/2025, 10:15
  3. 3. Using galactic neutrinos for constraining Lorentz Invariance Violation
    Jelena Celic
    28/07/2025, 10:30
  4. 4. TBD
    Annette Bremer (Universität Würzburg)
    28/07/2025, 10:45
  5. 5. XMM-Newton Analysis of SNR J0406-7009
    Edwin John Anthikat
    28/07/2025, 11:30
  6. 6. The IceCube Upgrade
    Anna Eimer
    28/07/2025, 11:45
  7. 17. Constraining the Physics of Very-High-Energy Emission in Blazars through High-Frequency Radio Monitoring
    Florian Eppel (JMU Würzburg)
    28/07/2025, 12:00
  8. 8. Hot subdwarf stars from the Hamburg Quasar survey
    Lennard Kufleitner
    28/07/2025, 13:45
  9. 9. Search for Axion-like Particles from Massive Stars
    Saurabh Mittal
    28/07/2025, 14:00
  10. 10. Detecting extensive air showers with SKA-low
    Philipp Laub (Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander-Universität Erlangen-Nürnberg)
    28/07/2025, 14:15
  11. 11. Spectral Behavior of Cepheus X-4 at Low Luminosity: Cyclotron Line Analysis Challenged by NuSTAR Instrumental Background
    Deniz Demirci
    28/07/2025, 15:00
  12. 12. Joint searches for neutrinos from the galactic plane with KM3NeT and IceCube
    Anke Mosbrugger
    28/07/2025, 15:15
  13. 13. High-energy Gamma ray astronomy in Würzburg - from Lightcurves to Skymaps
    Patrick Günther
    28/07/2025, 15:30
  14. 14. Raytracing in the SIXTE Simulator
    Neo Reinmann
    28/07/2025, 16:15
  15. 15. TBD
    Markus Pirke (ECAP)
    28/07/2025, 16:30
  16. 16. Probing the physics of jet launching and propagation through numerical simulations
    Ainara Saiz Pérez (Julius-Maximilians-Universität Würzburg)
    28/07/2025, 16:45
  17. 18. Constraining the Physics of Very-High-Energy Emission in Blazars through Radio Monitoring observations
    Florian Eppel (JMU Würzburg)