{ "id": "2308.00024", "version": "v1", "published": "2023-07-31T18:00:01.000Z", "updated": "2023-07-31T18:00:01.000Z", "title": "Searching for High-Energy Neutrino Emission from Seyfert Galaxies in the Northern Sky with IceCube", "authors": [ "Theo Glauch", "Ali Kheirandish", "Tomas Kontrimas", "Qinrui Liu", "Hans Niederhausen" ], "comment": "11 pages, 3 figures. Presented at the 38th International Cosmic Ray Conference (ICRC2023). See arXiv:2307.13047 for all IceCube contributions", "categories": [ "astro-ph.HE", "hep-ph" ], "abstract": "The recent detection of TeV neutrino emission from the nearby active galaxy NGC 1068 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 2.7$\\sigma$ significance, and at the same time constrain the collective neutrino emission from our source list.", "revisions": [ { "version": "v1", "updated": "2023-07-31T18:00:01.000Z" } ], "analyses": { "keywords": [ "high-energy neutrino emission", "seyfert galaxies", "northern sky", "generic single power-law spectral assumption", "total high-energy cosmic neutrino flux" ], "tags": [ "conference paper" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }