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BEGIN:VEVENT
DTSTAMP:20260522T133827Z
UID:https://www.ipp.mpg.de/events/41897/5593513
DTSTART:20250522T083000Z
DTEND:20250522T100000Z
CLASS:PUBLIC
CREATED:20250520T065922Z
DESCRIPTION:Abstract: The detection of a flux of TeV neutrinos from the nea
 rby Seyfert galaxy NGC1068 is particularly intriguing. The neutrino flux m
 easured by the IceCube neutrino observatory is at least two orders of magn
 itude higher than its gamma-ray counterpart\, in contrast with the hypothe
 sis of correlation between high-energy neutrinos and gamma-rays in AGN. Th
 is finding motivated further searches for neutrino emission in sources sim
 ilar to NGC 1068. This source is among the brightest X-ray Seyfert galaxie
 s\, supporting models that suggest that high-energy neutrinos are produced
  in the vicinity of the supermassive black hole\, most likely in the AGN c
 orona. I will present the most recent IceCube results on searches for neut
 rino sources\, including both a follow-up of already published results and
  findings on a newly compiled list of X-ray bright non-blazars AGN. In par
 ticular\, we confirm the measurement of a neutrino flux from NGC1068\, and
  we report the evidence of neutrino emission from a subset of 11 X-ray bri
 ght AGN at a 3.3σ level.\nVortragende(r): Elena Manao
LAST-MODIFIED:20250520T070017Z
LOCATION:IPP L7A\, Raum: 121
ORGANIZER;CN=Plasma Astrophysics group (TOK):mailto:artem.bohdan@ipp.mpg.de
SUMMARY:Neutrino Emission from X-ray Bright Active Galactic Nuclei: a revie
 w of recent IceCube results
URL;VALUE=URI:https://www.ipp.mpg.de/events/41897/5593513
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