Home > Publications database > Search for neutrino emission from hard X-ray AGN with IceCube > print

001     617514
005     20260111053254.0
024 7 _ |a Abbasi:2024hwv
|2 INSPIRETeX
024 7 _ |a inspire:2797004
|2 inspire
024 7 _ |a arXiv:2406.06684
|2 arXiv
024 7 _ |a altmetric:164466235
|2 altmetric
037 _ _ |a PUBDB-2024-06845
041 _ _ |a English
088 _ _ |a arXiv:2406.06684
|2 arXiv
100 1 _ |a Abbasi, R.
|b 0
245 _ _ |a Search for neutrino emission from hard X-ray AGN with IceCube
260 _ _ |c 2024
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1732281073_2691934
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
520 _ _ |a Active Galactic Nuclei (AGN) are promising candidate sources of high-energy astrophysical neutrinos since they provide environments rich in matter and photon targets where cosmic ray interactions may lead to the production of gamma rays and neutrinos. We searched for high-energy neutrino emission from AGN using the $\textit{Swift}$-BAT Spectroscopic Survey (BASS) catalog of hard X-ray sources and 12 years of IceCube muon track data. First, upon performing a stacked search, no significant emission was found. Second, we searched for neutrinos from a list of 43 candidate sources and found an excess from the direction of two sources, Seyfert galaxies NGC 1068 and NGC 4151. We observed NGC 1068 at flux $\phi_{\nu_{\mu}+\bar{\nu}_{\mu}}$ = $4.02_{-1.52}^{+1.58} \times 10^{-11}$ TeV$^{-1}$ cm$^{-2}$ s$^{-1}$ normalized at 1 TeV, with power-law spectral index, $\gamma$ = 3.10$^{+0.26}_{-0.22}$, consistent with previous IceCube results. The observation of a neutrino excess from the direction of NGC 4151 is at a post-trial significance of 2.9$\sigma$. If interpreted as an astrophysical signal, the excess observed from NGC 4151 corresponds to a flux $\phi_{\nu_{\mu}+\bar{\nu}_{\mu}}$ = $1.51_{-0.81}^{+0.99} \times 10^{-11}$ TeV$^{-1}$ cm$^{-2}$ s$^{-1}$ normalized at 1 TeV and $\gamma$ = 2.83$^{+0.35}_{-0.28}$.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to INSPIRE
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
|e IceCube South Pole Neutrino Observatory
|x 0
700 1 _ |a Ackermann, M.
|b 1
700 1 _ |a Adams, J.
|b 2
700 1 _ |a Agarwalla, S. K.
|0 P:(DE-HGF)0
|b 3
|e Corresponding author
700 1 _ |a Aguilar, J. A.
|b 4
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|b 6
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|b 8
700 1 _ |a Argüelles, C.
|b 9
700 1 _ |a Ashida, Y.
|b 10
700 1 _ |a Athanasiadou, S.
|0 P:(DE-H253)PIP1097003
|b 11
|u desy
700 1 _ |a Ausborm, L.
|b 12
700 1 _ |a Axani, S. N.
|b 13
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|b 14
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700 1 _ |a Blot, S.
|0 P:(DE-H253)PIP1027576
|b 32
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|0 P:(DE-H253)PIP1092168
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|0 P:(DE-H253)PIP1106871
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700 1 _ |a Weigel, P.
|b 400
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700 1 _ |a Wendt, C.
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700 1 _ |a Werthebach, J.
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700 1 _ |a Weyrauch, M.
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700 1 _ |a Whitehorn, N.
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700 1 _ |a Yu, S.
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Marc 21