IceCube Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies

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  • uploaded June 26, 2021

Discussion timeslot (ZOOM-Meeting): 19. July 2021 - 18:00
ZOOM-Meeting URL: https://desy.zoom.us/j/91999581729
ZOOM-Meeting ID: 91999581729
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/39-Astrophysical-Neutrinos-Theoretical-amp-Experimental-Results-NU/70
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-05/6

Abstract:
'With infrared luminosities $L_{mathrm{IR}} geq 10^{12} L_{odot}$, Ultra-Luminous Infrared Galaxies (ULIRGs) are the most luminous objects in the infrared sky. They are predominantly powered by starburst regions with star-formation rates $ larger sim 100~ M_{odot}~ mathrm{yr^{-1}}$. ULIRGs can also host an active galactic nucleus (AGN). Both the starburst and AGN environments contain plausible hadronic accelerators, making ULIRGs candidate neutrino sources. We present the results of an IceCube stacking analysis searching for high-energy neutrinos from a representative sample of 75 ULIRGs with $z leq 0.13$. While no significant excess of ULIRG neutrinos is found in 7.5 years of IceCube data, upper limits are reported on the neutrino flux from these 75 ULIRGs as well as the full ULIRG source population. In addition, constraints are provided on models predicting neutrino emission from ULIRGs.'

Authors: Pablo Correa | Krijn de Vries | Nick van Eijndhoven | For the IceCube Collaboration
Collaboration: IceCube

Indico-ID: 457
Proceeding URL: https://pos.sissa.it/395/1115

Tags:
Presenter: Pablo Correa

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