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The IceCube Neutrino Observatory opened the window on high-energy neutrino astronomy by confirming the existence of PeV astrophysical neutrinos and identifying the first compelling astrophysical neutrino source in the blazar TXS0506+056.…

High Energy Astrophysical Phenomena · Physics 2021-07-20 Brian Clark , Robert Halliday

We present first neutrino induced events observed with a deep underwater neutrino telescope. Data from 70 days effective life time of the BAIKAL prototype telescope NT-96 have been analyzed with two different methods. With the standard…

Astrophysics · Physics 2008-11-26 Baikal Collaboration , V. A. Balkanov et al

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will host the next generation Cherenkov neutrino telescope and nodes for a deep sea multidisciplinary observatory, providing oceanographers, marine…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Annarita Margiotta

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

We present a fast data processing system for the Baikal-GVD neutrino telescope, designed for rapid identification of astrophysical neutrino events. Leveraging Baikal-GVD's modular cluster architecture, the system implements parallelized…

T2K is a long baseline neutrino experiment, entering Phase II with a Near Detector upgrade. The T2K near detector (ND280) upgrade consists of the installation of three new detector systems: a plastic scintillator neutrino active target…

The study of neutrino oscillation at accelerators is limited by systematic uncertainties, in particular on the neutrino flux, cross-section, and energy estimates. These systematic uncertainties could be eliminated by a novel experimental…

A new EAS Cherenkov light array, Tunka-133, with ~1 km^2 geometrical area has been installed at the Tunka Valley (50 km from Lake Baikal) in 2009. The array permits a detailed study of cosmic ray energy spectrum and mass composition in the…

This document presents the physics case for bringing SciBar, the fully active, finely segmented tracking detector at KEK, to the FNAL Booster Neutrino Beam (BNB) line. This unique opportunity arose with the termination of K2K beam…

High Energy Physics - Experiment · Physics 2012-08-27 SciBooNE Collaboration

We report on the observation of a rare neutrino event detected by Baikal-GVD in April 2021. The event GVD210418CA is the highest-energy cascade observed by Baikal-GVD so far from the direction below the horizon. The estimated cascade energy…

The KArlsruhe TRItium Neutrino (KATRIN) experiment, which aims to make a direct and model-independent determination of the absolute neutrino mass scale, is a complex experiment with many components. More than 15 years ago, we published a…

Instrumentation and Detectors · Physics 2021-09-01 M. Aker , K. Altenmüller , J. F. Amsbaugh , M. Arenz , M. Babutzka , J. Bast , S. Bauer , H. Bechtler , M. Beck , A. Beglarian , J. Behrens , B. Bender , R. Berendes , A. Berlev , U. Besserer , C. Bettin , B. Bieringer , K. Blaum , F. Block , S. Bobien , J. Bohn , K. Bokeloh , H. Bolz , B. Bornschein , L. Bornschein , M. Böttcher , H. Bouquet , N. M. Boyd , T. Brunst , T. H. Burritt , T. S. Caldwell , Z. Chaoui , S. Chilingaryan , W. Choi , T. J. Corona , G. A. Cox , K. Debowski , M. Deffert , M. Descher , D. Díaz Barrero , P. J. Doe , O. Dragoun , G. Drexlin , J. A. Dunmore , S. Dyba , F. Edzards , F. Eichelhardt , K. Eitel , E. Ellinger , R. Engel , S. Enomoto , M. Erhard , D. Eversheim , M. Fedkevych , A. Felden , S. Fischer , J. A. Formaggio , F. M. Fränkle , G. B. Franklin , H. Frenzel , F. Friedel , A. Fulst , K. Gauda , R. Gehring , W. Gil , F. Glück , S. Görhardt , J. Grimm , S. Grohmann , S. Groh , R. Grössle , R. Gumbsheimer , M. Hackenjos , D. Häßler , V. Hannen , F. Harms , G. C. Harper , J. Hartmann , N. Haußmann , F. Heizmann , K. Helbing , M. Held , S. Hickford , D. Hilk , B. Hillen , R. Hiller , D. Hillesheimer , D. Hinz , T. Höhn , S. Holzmann , S. Horn , M. Hötzel , T. Houdy , M. A. Howe , A. Huber , T. James , A. Jansen , M. Kaiser , C. Karl , O. Kazachenko , J. Kellerer , L. Kippenbrock , M. Kleesiek , M. Kleifges , J. Kleinfeller , M. Klein , L. Köllenberger , A. Kopmann , M. Korzeczek , A. Kosmider , A. Kovalík , B. Krasch , H. Krause , M. Kraus , L. Kuckert , A. Kumb , N. Kunka , T. Lasserre , L. La Cascio , O. Lebeda , M. L. Leber , B. Lehnert , B. Leiber , J. Letnev , R. J. Lewis , T. L. Le , S. Lichter , A. Lokhov , J. M. Lopez Poyato , M. Machatschek , E. Malcherek , M. Mark , A. Marsteller , E. L. Martin , K. Mehret , M. Meloni , C. Melzer , A. Menshikov , S. Mertens , L. I. Minter , B. Monreal , J. Mostafa , K. Müller , A. W. Myers , U. Naumann , H. Neumann , S. Niemes , P. Oelpmann , A. Off , H. -W. Ortjohann , A. Osipowicz , B. Ostrick , D. S. Parno , D. A. Peterson , P. Plischke , A. W. P. Poon , M. Prall , F. Priester , P. C. -O. Ranitzsch , J. Reich , P. Renschler , O. Rest , R. Rinderspacher , R. G. H. Robertson , W. Rodejohann , C. Rodenbeck , P. Rohr , M. Röllig , C. Röttele , S. Rupp , M. Ryšavý , R. Sack , A. Saenz , M. Sagawe , P. Schäfer , A. Schaller , L. Schimpf , K. Schlösser , M. Schlösser , L. Schlüter , S. Schneidewind , H. Schön , K. Schönung , M. Schrank , B. Schulz , J. Schwarz , M. Šefčík , H. Seitz-Moskaliuk , W. Seller , V. Sibille , D. Siegmann , M. Slezák , F. Spanier , M. Steidl , M. Sturm , M. Sun , D. Tcherniakhovski , H. H. Telle , L. A. Thorne , T. Thümmler , N. Titov , I. Tkachev , N. Trost , K. Valerius , B. A. VanDevender , T. D. Van Wechel , D. Vénos , A. Verbeek , R. Vianden , A. P. Vizcaya Hernández , K. Vogt , B. L. Wall , N. Wandkowsky , M. Weber , H. Weingardt , C. Weinheimer , C. Weiss , S. Welte , J. Wendel , K. J. Wierman , J. F. Wilkerson , J. Wolf , S. Wüstling , W. Xu , Y. -R. Yen , M. Zacher , S. Zadoroghny , M. Zboril , G. Zeller

The KEK-to-Kamioka long-baseline neutrino experiment (K2K) has begun its investigation of neutrino oscillation, and has established the method of a long-baseline neutrino experiment. From the first 100 days of data-taking, a deficit of muon…

High Energy Physics - Experiment · Physics 2007-05-23 Takanobu Ishii

We present the results of a search for high energy extraterrestrial neutrinos with the Baikal underwater Cherenkov detector NT200, based on data taken in 1998 - 2002. Upper limits on the diffuse fluxes of $\nu_e+\nu_{\mu}+\nu_{\tau}$,…

Astrophysics · Physics 2019-08-14 V. Aynutdinov

We present the results of a search for high energy extraterrestrial neutrinos with the Baikal underwater Cherenkov detector NT200, based on data taken in 1998 - 2002 (1038 live days).Upper limits on the diffuse fluxes of…

Astrophysics · Physics 2019-08-14 R. Wischnewski

The K2K Long--Baseline neutrino oscillation experiment has been aquiring data since mid-1999 and has analysed those up to March of 2001. Forty-four fully contained events are observedin the fiducial volume of the far detector where…

High Energy Physics - Experiment · Physics 2019-08-14 James E. Hill

T2K is a long baseline high intensity neutrino oscillation experiment employing an off-axis design to search for the as yet unobserved appearance of \nu_e neutrinos in a \nu_{\mu} beam. The neutrino beam originates at the J-PARC facility in…

High Energy Physics - Experiment · Physics 2019-08-14 Mark Hartz

High-energy neutrino astronomy has advanced rapidly in recent years, with IceCube, KM3NeT, and Baikal-GVD establishing a diffuse astrophysical flux and pointing to promising source candidates. These achievements mark the transition from…

Instrumentation and Methods for Astrophysics · Physics 2025-10-29 Iwan Morton-Blake , Fuyudi Zhang , Qichao Chang , Shuhua Hao , Weilun Huang , Hualin Mei , Wei Tian , Yingwei Wang , Xin Xiang , Donglian Xu

We discuss the discovery potential of extended very-high-energy (VHE) neutrino sources by the future KM3 Neutrino Telescope (KM3NeT) in the context of the constraining power of the Cherenkov Telescope Array (CTA), designed for deep surveys…

High Energy Astrophysical Phenomena · Physics 2018-04-04 Lucia Ambrogi , Silvia Celli , Felix Aharonian

The IceCube Neutrino Observatory is an array of 5,160 photomultipliers (PMTs) deployed on 86 strings at 1.5-2.5 km depth within the ice at the South Pole. The main goal of the IceCube experiment is the detection of an astrophysical neutrino…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Juan A. Aguilar