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Related papers: High-Energy Neutrino Emission from Blazars

200 papers

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

The IceCube Neutrino Observatory has detected several hundred high-energy neutrinos from cosmic sources. Despite numerous studies searching for their origin, it is still not known which sources emit them. A few likely individual…

High Energy Astrophysical Phenomena · Physics 2026-04-29 Pouya M. Kouch , Talvikki Hovatta , Elina Lindfors , Ioannis Liodakis , Karri I. I. Koljonen , Alessandro Paggi

Blazars are a rare class of active galactic nuclei (AGN) with relativistic jets pointing towards the observer. Jets are thought to be launched as Poynting-flux dominated outflows that accelerate to relativistic speeds at the expense of the…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Maria Petropoulou , Filippos Psarras , Dimitrios Giannios

We explore the correlation of $\gamma$-ray emitting blazars with IceCube neutrinos by using three very recently completed, and independently built, catalogues and the latest neutrino lists. We introduce a new observable, namely the number…

High Energy Astrophysical Phenomena · Physics 2016-02-03 P. Padovani , E. Resconi , P. Giommi , B. Arsioli , Y. L. Chang

Gamma-ray-bright active galactic nuclei (AGN) have been one of the most promising source classes of high-energy astrophysical neutrinos detected by IceCube. The first evidence of an IceCube point source was a blazar detected by the Fermi…

High Energy Astrophysical Phenomena · Physics 2025-07-10 Sam Hori , Abhishek Desai , Justin Vandenbroucke

The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The background due to atmospheric particles can be drastically…

High Energy Astrophysical Phenomena · Physics 2016-08-08 S. Adrián-Martínez , A. Albert , M. André , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bogazzi , R. Bormuth , M. Bou-Cabo , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , T. Chiarusi , M. Circella , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , I. Dekeyser , A. Deschamps , G. De Bonis , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , A. Dumas , T. Eberl , D. Elsässer , A. Enzenhöfer , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , R. Gracia-Ruiz , K. Graf , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , A. Herrero , J. Hößl , J. Hofestädt , C. Hugon , C. W James , M. de Jong , M. Kadler , O. Kalekin , U. Katz , D. Kießling , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , G. Lambard , D. Lattuada , D. Lefèvre , E. Leonora , S. Loucatos , S. Mangano , A. Margiotta , J. A. Martínez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , M. Neff , E. Nezri , G. E. Păvălaş , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldaña , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sánchez-Losa , M. Taiuti , C. Tamburini , A. Trovato , M. Tselengidou , C. Tönnis , D. Turpin , B. Vallage , C. Vallée , V. Van Elewyck , E. Visser , D. Vivolo , S. Wagner , J. Wilms , J. D. Zornoza , J. Zúñiga

We discuss the fluxes of high energy neutrinos and gamma-rays expected from AGNs if hadrons can be effectively accelerated to ultra-high energies by their relativistic jets, as currently believed. Fluxes of multi-TeV neutrinos detectable by…

Astrophysics · Physics 2009-11-10 A. Atoyan , C. D. Dermer

There is mounting evidence that ultra-energetic neutrinos of astrophysical origin may be associated with blazars. Here we investigate a unique sample of 47 blazars, $\sim 20$ of which could be new neutrino sources. In particular, we focus…

High Energy Astrophysical Phenomena · Physics 2021-04-21 Simona Paiano , Renato Falomo , Aldo Treves , Paolo Padovani , Paolo Giommi , Riccardo Scarpa

The IceCube neutrino observatory, a cubic-kilometer particle detector at the South Pole, first announced the discovery of an astrophysical flux of high-energy neutrinos in the TeV-PeV range in 2013, followed in 2017 by the detection of a…

High Energy Astrophysical Phenomena · Physics 2019-08-15 Marcos Santander

Observational information on high-energy astrophysical neutrinos is being continuously collected by the IceCube observatory. However, the sources of neutrinos are still unknown. In this study, we use radio very-long-baseline interferometry…

High Energy Astrophysical Phenomena · Physics 2020-09-10 A. V. Plavin , Y. Y. Kovalev , Y. A. Kovalev , S. V. Troitsky

The evidence for joint gamma and neutrino emission from the blazar TXS 0506+056 has renewed interest in blazars as neutrino sources. The detection of neutrinos from blazars can be seen as the smoking gun for the presence of relativistic…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Matteo Cerruti

Active Galactic Nuclei (AGN) are believed to be one of the main source candidates for the high-energy (TeV-PeV) cosmic neutrino flux recently discovered by the IceCube neutrino observatory. Nevertheless, several correlation studies between…

High Energy Astrophysical Phenomena · Physics 2016-11-23 G. Maggi , S. Buitink , P. Correa , K. D. de Vries , G. Gentile , J. Leon Tavares , O. Scholten , N. van Eijndhoven , M. Vereecken , T. Winchen

Protons accelerated in the cores of active galactic nuclei can effectively produce neutrinos only if the soft radiation background in the core is sufficiently high. We find restrictions on the spectral properties and luminosity of blazars…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. Yu. Neronov , D. V. Semikoz

Gamma-ray blazars are among the most extreme astrophysical sources, harboring phenomena far more energetic than those attainable by terrestrial accelerators. These galaxies are understood to be active galactic nuclei that are powered by…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Amy Furniss

The field of high-energy neutrino astronomy is undergoing a rapid evolution. After the discovery of a diffuse flux of astrophysical TeV-PeV neutrinos in 2013, the IceCube observatory has recently found first compelling evidence for neutrino…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Markus Ahlers

The IceCube Neutrino Observatory has identified several individual neutrino emitters associated with supermassive black hole accretion phenomena, including blazars, tidal disruption events, and, unexpectedly, Seyfert galaxies. A key open…

High Energy Astrophysical Phenomena · Physics 2025-11-24 Shuying Zhou , Mouyuan Sun , Guobin Mou , Da-bin Lin , Tong Liu , Ming-Xuan Lu , Yongquan Xue

An updated analysis of a targeted search for high-energy neutrinos from Markarian 421 and Markarian 501 is reported. They are two of the closest and brightest extragalactic sources in the TeV band. In contrast to other types of active…

High Energy Astrophysical Phenomena · Physics 2019-11-13 Mukharbek Organokov , Thierry Pradier

We review and discuss recent results on the search for correlations between astrophysical neutrinos and gamma-ray-detected sources, with many extra-galactic studies reporting potential associations with different types of blazars. We…

High Energy Astrophysical Phenomena · Physics 2021-12-14 Paolo Giommi , Paolo Padovani

Blazars are the most violent steady/recurrent sources of high-energy gamma-ray emission in the known Universe. They are prominent emitters of electromagnetic radiation throughout the entire electromagnetic spectrum. The observable radiation…

Astrophysics · Physics 2008-11-26 Markus Boettcher

A correlation between the highest energy Cosmic Rays (above ~ EeV) and the distribution of active galactic nuclei (AGN) gives rise to a prediction of neutrino production in the same sources. In this paper, we present a detailed AGN model,…

Astrophysics · Physics 2009-11-13 Julia K. Becker , Peter L. Biermann