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Enrico Peretti17/06/2026, 12:00Talk
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Sweta Menon (Istituto Nazionale di Astrofisica (INAF))17/06/2026, 12:30Talk
Seyfert galaxies have emerged as the most promising counterparts to TeV neutrino excesses detected by IceCube, with significant associations above the 3σ level. Stacked analyses of X-ray bright AGN further indicate a collective signal at ~3σ, supporting their contribution to the multi-messenger neutrino sky.
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The AGN environment provides multiple sites capable of accelerating protons to the... -
Gaia Delucchi (Istituto Nazionale di Astrofisica (INAF))17/06/2026, 12:45Talk
Blazars are a class of AGN characterised by relativistic jets pointed towards our LoS. Traditionally, they are classified into two families: BL Lacs (no emission lines suggesting an inefficient accretion flow and faint bluer broad band SEDs) and FSRQs (strong emission lines, radiatively efficient accretion and brighter red SEDs). However, recent studies have highlighted that blazars identified...
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Stefano Gabici17/06/2026, 15:00Talk
I will briefly review our knowledge on extragalactic cosmic rays. I will then discuss the possibility that these particles are accelerated at AGNi, and discuss the multi-messenger signals that unavoidably accompany particle accelerator in these objects.
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