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We investigate whether the emission of neutrinos observed in 2014-15 from the direction of the blazar TXS 0506+056 can be accommodated with leptohadronic multi-wavelength models of the source commonly adopted for the 2017 flare. While…

High Energy Astrophysical Phenomena · Physics 2019-04-17 Xavier Rodrigues , Shan Gao , Anatoli Fedynitch , Andrea Palladino , Walter Winter

The blazars are one of the leading candidate sources of high-energy neutrinos. Recently, two blazars have been found to be temporally and spatially correlated with some IceCube high-energy neutrino events. The two blazars, GB6 J2113+1121…

High Energy Astrophysical Phenomena · Physics 2025-05-08 Xiong Jiang , Neng-Hui Liao , Xue Rui , Yi-Zhong Fan , Da-Ming Wei

On July 30th, 2019 IceCube detected a high-energy astrophysical muon neutrino candidate, IC-190730A, with a $67\%$ probability of astrophysical origin. The flat spectrum radio quasar (FSRQ) PKS 1502+106 is in the error circle of the…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Foteini Oikonomou , Maria Petropoulou , Kohta Murase , Aaron Tohuvavohu , Georgios Vasilopoulos , Sara Buson , Marcos Santander

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…

We present a multi-wavelength study of a blazar PKS 0446+11, motivated by its spatial association with the neutrino event IC240105A detected by the IceCube Neutrino Observatory on 2024 January 5. The source is located 0.4 degrees from the…

High Energy Astrophysical Phenomena · Physics 2026-02-04 Rukaiya Khatoon , Markus Boettcher , Joshua Robinson

The blazar PKS 0735+178 is possibly associated with multiple neutrino events observed by the IceCube, Baikal, Baksan, and KM3NeT neutrino telescopes while it was flaring in the $\gamma$-ray, X-ray, ultraviolet and optical bands. We present…

High Energy Astrophysical Phenomena · Physics 2022-12-21 N. Sahakyan , P. Giommi , P. Padovani , M. Petropoulou , D. Bégué , B. Boccardi , S. Gasparyan

There is mounting evidence that blazars are the sources of part of the very-high-energy astrophysical neutrino flux detected by IceCube. In particular, there have been several spatial and temporal coincidences of individual IceCube neutrino…

High Energy Astrophysical Phenomena · Physics 2024-10-30 Joshua Robinson , Markus Boettcher

We report on multiwavelength target-of-opportunity observations of the blazar PKS 0735+178, located 2.2 degrees away from the best-fit position of the IceCube neutrino event 211208A. The source was in a high-flux state in the optical,…

High Energy Astrophysical Phenomena · Physics 2023-08-16 M. Pohl , K. Mori

We consider implications of high-energy neutrino emission from blazar flares, including the recent event IceCube-170922A and the 2014-2015 neutrino flare that could originate from TXS 0506+056. First, we discuss their contribution to the…

High Energy Astrophysical Phenomena · Physics 2018-10-11 Kohta Murase , Foteini Oikonomou , Maria Petropoulou

We report on multiwavelength target-of-opportunity observations of the blazar PKS 0735+178, located 2.2$^\circ$ away from the best-fit position of the IceCube neutrino event IceCube-211208A detected on December 8, 2021. The source was in a…

High Energy Astrophysical Phenomena · Physics 2023-07-03 A. Acharyya , C. B. Adams , A. Archer , P. Bangale , J. T. Bartkoske , P. Batista , W. Benbow , A. Brill , J. H. Buckley , J. L. Christiansen , A. J. Chromey , M. Errando , A. Falcone , Q. Feng , G. M. Foote , L. Fortson , A. Furniss , G. Gallagher , W. Hanlon , D. Hanna , O. Hervet , C. E. Hinrichs , J. Hoang , J. Holder , T. B. Humensky , W. Jin , P. Kaaret , M. Kertzman , M. Kherlakian , D. Kieda , T. K. Kleiner , N. Korzoun , S. Kumar , M. J. Lang , M. Lundy , G. Maier , C. E McGrath , M. J. Millard , J. Millis , C. L. Mooney , P. Moriarty , R. Mukherjee , S. O'Brien , R. A. Ong , M. Pohl , E. Pueschel , J. Quinn , K. Ragan , P. T. Reynolds , D. Ribeiro , E. Roache , I. Sadeh , A. C. Sadun , L. Saha , M. Santander , G. H. Sembroski , R. Shang , M. Splettstoesser , A. Kaushik Talluri , J. V. Tucci , V. V. Vassiliev , A. Weinstein , D. A. Williams , S. L. Wong , J. Woo , F. Aharonian , J. Aschersleben , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlohr , B. Bi , M. Bottcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , M. Bouyahiaoui , F. Bradascio , M. Breuhaus , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caroff , S. Casanova , R. Cecil , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , S. Dai , J. Damascene Mbarubucyeye , A. Djannati-Atai , A. Dmytriiev , V. Doroshenko , S. Einecke , J. -P. Ernenwein , G. Fichet de Clairfontaine , M. Filipovic , G. Fontaine , M. Fussling , S. Funk , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , P. Goswami , G. Grolleron , L. Haerer , J. A. Hinton , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynski , R. Khatoon , B. Khelifi , S. Klepser , W. Kluzniak , K. Kosack , D. Kostunin , R. G. Lang , S. Le Stum , A. Lemiere , J. P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Marti-Devesa , R. Marx , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , T. Murach , K. Nakashima , J. Niemiec , A. Priyana Noel , P. O'Brien , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , G. Peron , D. A. Prokhorov , G. Puhlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , H. Ren , M. Renaud , F. Rieger , B. Rudak , E. Ruiz-Velasco , V. Sahakian , A. Santangelo , M. Sasaki , J. Schafer , F. Schussler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , A. Specovius , S. Spencer , L. Stawarz , R. Steenkamp , S. Steinmassl , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , R. Terrier , C. van Eldik , M. Vecchi , J. Veh , C. Venter , J. Vink , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zouari , N. Zywucka , K. Mori

The origin of the diffuse astrophysical neutrino flux observed by the IceCube experiment is still under debate. In recent years there have been associations of neutrino events with individual blazars, which are active galaxies with…

High Energy Astrophysical Phenomena · Physics 2024-03-05 Xavier Rodrigues , Vaidehi S. Paliya , Simone Garrappa , Anastasiia Omeliukh , Anna Franckowiak , Walter Winter

Blazars are interesting source candidates for astrophysical neutrino emission. Multi-messenger lepto-hadronic models based on proton-photon (p-gamma) interactions result in predictions for the neutrino spectra (''p-gamma spectra'') which…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Julian Kuhlmann , Francesca Capel

Detection of the IceCube-170922A neutrino coincident with the flaring blazar TXS 0506+056, the first and only 3-sigma high-energy neutrino source association to date, offers a potential breakthrough in our understanding of high-energy…

In September 2017, the IceCube Neutrino Observatory recorded a very-high-energy neutrino in directional coincidence with a blazar in an unusually bright gamma-ray state, TXS0506+056. Blazars are prominent photon sources in the universe…

High Energy Astrophysical Phenomena · Physics 2019-05-14 Shan Gao , Anatoli Fedynitch , Walter Winter , Martin Pohl

A correlation has been reported between the arrival directions of high-energy IceCube events and gamma-ray blazars classified as intermediate- and high-synchrotron-peaked BL Lacs. Subsequent studies have investigated the optical properties…

High Energy Astrophysical Phenomena · Physics 2024-11-07 Xavier Rodrigues , Martina Karl , Paolo Padovani , Paolo Giommi , Simona Paiano , Renato Falomo , Maria Petropoulou , Foteini Oikonomou

The IceCube collaboration reported a $\sim 3.5\sigma$ excess of $13\pm5$ neutrino events in the direction of the blazar TXS 0506+56 during a $\sim$6 month period in 2014-2015, as well as the ($\sim3\sigma$) detection of a high-energy muon…

High Energy Astrophysical Phenomena · Physics 2020-02-03 B. Theodore Zhang , Maria Petropoulou , Kohta Murase , Foteini Oikonomou

Motivated by the recently reported evidence of an association between a high-energy neutrino and a gamma-ray flare from the blazar TXS 0506+056, we calculate the expected high-energy neutrino signal from past, individual flares, from twelve…

High Energy Astrophysical Phenomena · Physics 2019-09-23 Foteini Oikonomou , Kohta Murase , Paolo Padovani , Elisa Resconi , Peter Mészáros

A high-energy muon neutrino event, IceCube-170922A, was recently discovered in both spatial and temporal coincidence with a gamma-ray flare of the blazar TXS 0506+056. It has been shown, with standard one-zone models, that neutrinos can be…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Rui Xue , Ruo-Yu Liu , Maria Petropoulou , Foteini Oikonomou , Ze-Rui Wang , Kai Wang , Xiang-Yu Wang

The blazar TXS 0506+056 has been suggested to be a potential high-energy neutrino source thanks to the observations of IceCube, which found outburst-like neutrino emissions during 2014-2015 and 2017 in the transient emission search, and a…

High Energy Astrophysical Phenomena · Physics 2025-09-19 Zhen-Jie Wang , Ruo-Yu Liu , Xiang-Yu Wang

The characteristic two-component blazar spectral energy distribution (SED) can be of either leptonic and/or hadronic origins. The potential association of the high-energy neutrino event IceCube-170922A with the flaring blazar TXS~0506+056…

High Energy Astrophysical Phenomena · Physics 2019-05-15 Haocheng Zhang , Ke Fang , Hui Li , Dimitrios Giannios , Markus Böttcher , Sara Buson
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