Events
1st PIER Science Slam
WPC Theoretical Physics Symposium 2021
International Cosmic Ray Conference 2021
1st PIER Science Slam
WPC Theoretical Physics Symposium 2021
International Cosmic Ray Conference 2021
69 views
2 likes
0 favorites
Discussion timeslot (ZOOM-Meeting): 12. July 2021 - 18:00
ZOOM-Meeting URL: https://desy.zoom.us/j/91896950007
ZOOM-Meeting ID: 91896950007
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/25-Blazars-AGN-MM/61
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-06/7
Abstract:
'On 22 September 2017 IceCube reported a high-energy neutrino event which was found to be coincident with a flaring blazar, TXS 0506+056. This first multi-messenger observation hinted at blazars being sources of observed high-energy astrophysical neutrinos and raised a need for extensive correlation studies. Recent work shows that the internal absorption of gamma rays, and their interactions intrinsic to the source and with the extragalactic background, will cause a lack of energetic gamma-ray and neutrino correlation while hinting towards a correlation between neutrinos and lower photon energy observations in the X-ray and radio bands. Studies based on published IceCube alerts and radio observations, report a possible radio-neutrino correlation in both gamma-ray bright and gamma-ray dim active galactic nuclei (AGN). However, they have marginal statistical significance due to limited available data. We present a correlation analysis between 15 GHz radio observations of AGN reported in the MOJAVE XV catalog and 10 years of IceCube detector data and discuss the results derived from a time averaged stacking analysis.'
Authors: Abhishek Desai
Co-Authors: Justin Vandenbroucke | Alex Pizzuto | For the IceCube Collaboration
Collaboration: IceCube
Indico-ID: 479
Proceeding URL: https://pos.sissa.it/395/949