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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202345958]

Issue
A&A
Volume 679, November 2023
Article Number C1
Number of page(s) 3
Section Astrophysical processes
DOI https://doi.org/10.1051/0004-6361/202345958e
Published online 03 November 2023

Erratum for: A&A 677, A53 (2023), https://doi.org/10.1051/0004-6361/202345958

We found the following misprints in the original manuscript:

  • In the Introduction, the correct name of the Seyfert galaxy referred to is NGC 1068.

  • In Eq. (1), there was a typo in the luminosity units, which should be erg s−1.

  • In Eq. (20), there was a missing minus sing in the last member on the right, that is, it should read as follows:

    b i , l o s s ′ = d E i ′ d t ′ | loss ≡ − E i ′ ∑ j t i , j ′ − 1 ( E i ′ ) . $$ \begin{aligned} b^{\prime }_{i,\mathrm loss}= \left.\frac{dE^{\prime }_i}{dt^{\prime }}\right|_{\rm loss}\equiv - E^{\prime }_i \sum _j t^{\prime -1}_{i,j}(E^{\prime }_{i}). \end{aligned} $$(20)

  • In the Acknowledgements section, the correct acronym for the financial support agency is ANPCyT.

Finally, Figs. (17) and (18) in the original paper correspond to a slightly different set of parameters than those presented in the paper. Therefore, we include below the correct versions of the above mentioned figures showing the flavor ratios obtained with the intergrated neutrino fluxes. The entirety of the discussion and conclusions remain valid as originallystated.

thumbnail Fig. 17.

Flavor ratios of the integrated fluxes of neutrinos with energy above Eν,min for L0 = 1050erg s−1 (left panels) and L0 = 1051erg s−1 (right panels). All plots are for Γ = 100. The top plots correspond to aep = 1 and the bottom ones to aep = 100. The green, orange, and blue curves correspond to the electron, muon, and tau flavor ratios, respectively. The long-dashed, solid, and short-dashed lines refer to the results for ϵB = 0.01, ϵB = 0.1, and ϵB = 1, respectively. The flavor ratios expected without considering losses are indicated with gray dotted lines for the electron flavor, gray long-dashed lines for the muon flavor, and gray long-short dashed lines for the tau flavor.

thumbnail Fig. 18.

Flavor ratios of the integrated fluxes of neutrinos with energy above Eν,min for L0 = 1050erg s−1 (left panels) and L0 = 1051erg s−1 (right panels). Both plots are for Γ = 100. The green, orange, and blue curves correspond to the electron, muon, and tau flavor ratios, respectively. The long-dashed, solid, and short-dashed lines refer to the results for ϵB = 0.01, ϵB = 0.1, and ϵB = 1, respectively. The flavor ratios expected without considering losses are indicated with gray dotted lines for the electron flavor, gray long-dashed lines for the muon flavor, and gray long-short dashed lines for the tau flavor.


© The Authors 2023

Licence Creative CommonsOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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All Figures

thumbnail Fig. 17.

Flavor ratios of the integrated fluxes of neutrinos with energy above Eν,min for L0 = 1050erg s−1 (left panels) and L0 = 1051erg s−1 (right panels). All plots are for Γ = 100. The top plots correspond to aep = 1 and the bottom ones to aep = 100. The green, orange, and blue curves correspond to the electron, muon, and tau flavor ratios, respectively. The long-dashed, solid, and short-dashed lines refer to the results for ϵB = 0.01, ϵB = 0.1, and ϵB = 1, respectively. The flavor ratios expected without considering losses are indicated with gray dotted lines for the electron flavor, gray long-dashed lines for the muon flavor, and gray long-short dashed lines for the tau flavor.
In the text
thumbnail Fig. 18.

Flavor ratios of the integrated fluxes of neutrinos with energy above Eν,min for L0 = 1050erg s−1 (left panels) and L0 = 1051erg s−1 (right panels). Both plots are for Γ = 100. The green, orange, and blue curves correspond to the electron, muon, and tau flavor ratios, respectively. The long-dashed, solid, and short-dashed lines refer to the results for ϵB = 0.01, ϵB = 0.1, and ϵB = 1, respectively. The flavor ratios expected without considering losses are indicated with gray dotted lines for the electron flavor, gray long-dashed lines for the muon flavor, and gray long-short dashed lines for the tau flavor.
In the text

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