Liu, Q.Abbasi, R.Ackermann, M.Adams, J.Agarwalla, S.K.Aguilar, J.A.Ahlers, M.Alameddine, J.M.Amin, N.M.Andeen, K.Anton, G.Argüelles, C.Ashida, Y.Athanasiadou, S.Axani, S.N.Bai, X.Balagopal, A.V.Baricevic, M.Barwick, S.W.Basu, V.et al.2025-12-022025-12-022024Proceedings of the 38th International Cosmic Ray Conference (ICRC 2023), as published in Proceedings of Science, 2024, vol.444, pp.1052-1-1052-111824-8039https://hdl.handle.net/2440/148386Published on: September 27, 2024The recent detection of TeVneutrino emission from the nearby active galaxyNGC1068 by IceCube suggests that AGN could make a sizable contribution to the total high-energy cosmic neutrino flux. The absence of TeV gamma rays from NGC 1068, indicates neutrino production originates in the innermost region of the AGN. Disk-corona models predict a correlation between neutrinos and keV X-rays in Seyfert galaxies, a subclass of AGN to which NGC 1068 belongs. Using 10 years of IceCube through-going track events, we report results from searches for neutrino signals from 27 additional sources in the Northern Sky by studying both the generic single power-law spectral assumption and spectra predicted by the disk-corona model. Our results show excesses of neutrinos associated with two sources, NGC 4151 and CGCG 420-015, at 2.7𝜎 significance, and at the same time constrain the collective neutrino emission from our source list.en© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).Conference paper10.22323/1.444.1052723921Burley, R.T. [0000-0002-6712-787X]Carnie-Bronca, E.G. [0000-0002-8195-5698]