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| 001 | 642881 | ||
| 005 | 20260113212143.0 | ||
| 024 | 7 | _ | |a 10.1051/0004-6361/202452143 |2 doi |
| 024 | 7 | _ | |a 0004-6361 |2 ISSN |
| 024 | 7 | _ | |a 1432-0746 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2409.04165 |2 arXiv |
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| 041 | _ | _ | |a English |
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| 088 | _ | _ | |a arXiv:2409.04165 |2 arXiv |
| 100 | 1 | _ | |a Omeliukh, A. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Multi-epoch leptohadronic modeling of neutrino source candidate blazar PKS 0735+178 |
| 260 | _ | _ | |a Les Ulis |c 2025 |b EDP Sciences |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 500 | _ | _ | |a A&A 695, A266 (2025). Accepted for publication in A&A |
| 520 | _ | _ | |a The origin of the astrophysical neutrino flux discovered by IceCube remains largely unknown. Several individual neutrino source candidates were observed. Among them is the gamma-ray flaring blazar TXS 0506+056. A similar coincidence of a high-energy neutrino and a gamma-ray flare was found in blazar PKS 0735+178. By modeling the spectral energy distributions of PKS 0735+178, we expect to investigate the physical conditions for neutrino production during different stages of the source activity. We analyze the multi-wavelength data during the selected periods of time. Using numerical simulations of radiation processes in the source, we study the parameter space of one-zone leptonic and leptohadronic models and find the best-fit solutions that explain the observed photon fluxes. We show the impact of model parameter degeneracy on the prediction of the neutrino spectra. We show that the available mutli-wavelength data are not sufficient to predict the neutrino spectrum unambiguously. Still, under the condition of maximal neutrino flux, we propose a scenario in which 0.2 neutrino events are produced during the 50 days flare. |
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| 700 | 1 | _ | |a Garrappa, S. |b 1 |
| 700 | 1 | _ | |a Fallah Ramazani, V. |b 2 |
| 700 | 1 | _ | |a Franckowiak, A. |0 P:(DE-H253)PIP1006092 |b 3 |
| 700 | 1 | _ | |a Winter, W. |0 P:(DE-H253)PIP1021242 |b 4 |
| 700 | 1 | _ | |a Lindfors, E. |b 5 |
| 700 | 1 | _ | |a Nilsson, K. |b 6 |
| 700 | 1 | _ | |a Jormanainen, J. |b 7 |
| 700 | 1 | _ | |a Wierda, F. |0 0000-0002-8657-0076 |b 8 |
| 700 | 1 | _ | |a Filippenko, A. V. |0 0000-0003-3460-0103 |b 9 |
| 700 | 1 | _ | |a Zheng, W. |b 10 |
| 700 | 1 | _ | |a Tornikoski, M. |0 0000-0003-1249-6026 |b 11 |
| 700 | 1 | _ | |a Lähteenmäki, A. |b 12 |
| 700 | 1 | _ | |a Kankkunen, S. |b 13 |
| 700 | 1 | _ | |a Tammi, J. |0 0000-0002-9164-2695 |b 14 |
| 773 | _ | _ | |a 10.1051/0004-6361/202452143 |g Vol. 695, p. A266 - |0 PERI:(DE-600)1458466-9 |p A266 |t Astronomy and astrophysics |v 695 |y 2025 |x 0004-6361 |
| 787 | 0 | _ | |a Omeliukh, A. et.al. |d 2025 |i IsParent |0 PUBDB-2026-00219 |r arXiv:2409.04165 |t Multi-epoch leptohadronic modeling of neutrino source candidate blazar PKS 0735+178 |
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