High Energy Phenomena in Relativistic Outflows (HEPRO) meeting.
WHEN: May 31 – June 4, 2027
WHERE: Palazzo de’ Toschi Bologna, Italy
Continuing a legacy that began in 2007, this 10th edition marks nearly two decades of advancing our understanding of the most energetic non-thermal phenomena in the Universe. HEPRO has established itself as the premier forum bringing together researchers working on extreme particle acceleration and relativistic outflows.
The Bologna meeting will highlight the immense progress made over the years. Discussions will center on:
- Jets and winds associated with supernova explosions
- Compact binaries containing accreting black holes or rotating neutron stars
- Relativistic electron–positron outflows from pulsars
- Gamma-ray burst (GRB) sources
- Relativistic jets extending from sub-parsec scales in blazars and quasars to multi-kiloparsec scales in active galactic nuclei (AGN)
Additionally, this event will serve as a meeting point for researchers worldwide to learn more about the progress of the Cherenkov Telescope Array Observatory (CTAO), both at a technological and scientific level.
Further details regarding registration, abstract submission, and the scientific program will be shared soon. In the meantime, you can check the website for updates: https://heprox.ctao.org/
If you have any questions, please feel free to reach out to us at hepro@cta-observatory.org.