Related papers: AURA - A radio frequency extension to IceCube

Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations

The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic…

High Energy Astrophysical Phenomena · Physics 2020-09-02 ARA Collaboration , P. Allison , S. Archambault , J. J. Beatty , M. Beheler-Amass , D. Z. Besson , M. Beydler , C. C. Chen , C. H. Chen , P. Chen , B. A. Clark , W. Clay , A. Connolly , L. Cremonesi , J. Davies , S. de Kockere , K. D. de Vries , C. Deaconu , M. Duvernois , E. Friedman , R. Gaior , J. Hanson , K. Hanson , K. D. Hoffman , B. Hokanson-Fasig , E. Hong , S. Y. Hsu , L. Hu , J. J. Huang , M. -H. Huang , K. Hughes , A. Ishihara , A. Karle , J. L. Kelley , R. Khandelwal , K. -C. Kim , M. -C. Kim , I. Kravchenko , K. Kurusu , H. Landsman , U. A. Latif , A. Laundrie , C. -J. Li , T. -C. Liu , M. -Y. Lu , B. Madison , K. Mase , T. Meures , J. Nam , R. J. Nichol , G. Nir , A. Novikov , A. Nozdrina , E. Oberla , A. O'Murchadha , J. Osborn , Y. Pan , C. Pfendner , J. Roth , P. Sandstrom , D. Seckel , Y. -S. Shiao , A. Shultz , D. Smith , J. Torres , J. Touart , N. van Eijndhoven , G. S. Varner , A. G. Vieregg , M. -Z. Wang , S. -H. Wang , S. A. Wissel , S. Yoshida , R. Young

Sensitivity studies for the IceCube-Gen2 radio array

The IceCube Neutrino Observatory at the South Pole has measured the diffuse astrophysical neutrino flux up to ~PeV energies and is starting to identify first point source candidates. The next generation facility, IceCube-Gen2, aims at…

High Energy Astrophysical Phenomena · Physics 2021-07-20 Steffen Hallmann , Brian Clark , Christian Glaser , Daniel Smith

Hybrid detection of high-energy cosmic neutrinos with the next-generation neutrino detectors at the South Pole

In 2013 the IceCube collaboration announced the discovery of a cosmic neutrino flux up to PeV energies, validating neutrino astronomy as the next promising observational technique to explore the high-energy Universe. The neutrino community…

High Energy Physics - Experiment · Physics 2019-08-27 S. Toscano , P. Coppin , K. D. de Vries , N. van Eijndhoven , J. A. Aguilar

Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array

Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that produce the highest energy cosmic rays by…

High Energy Astrophysical Phenomena · Physics 2010-02-02 Shang-Yu Sun , Pisin Chen , Melin Huang

The Study of a Cosmic Ray Candidate Detected by the Askaryan Radio Array

Experiments designed to detect ultra-high energy (UHE) neutrinos using radio techniques are also capable of detecting the radio signals from cosmic-ray (CR) induced air showers. These CR signals are important both as a background and as a…

Instrumentation and Methods for Astrophysics · Physics 2026-01-07 Shoukat Ali , Dave Z. Besson

Performance of the ARIANNA Hexagonal Radio Array

Installation of the ARIANNA Hexagonal Radio Array (HRA) on the Ross Ice Shelf of Antarctica has been completed. This detector serves as a pilot program to the ARIANNA neutrino telescope, which aims to measure the diffuse flux of very high…

Instrumentation and Methods for Astrophysics · Physics 2015-09-02 ARIANNA Collaboration , S. W. Barwick , E. C. Berg , D. Z. Besson , G. Binder , W. R. Binns , D. Boersma , R. G. Bose , D. L. Braun , J. H. Buckley , V. Bugaev , S. Buitink , K. Dookayka , P. F. Dowkontt , T. Duffin , S. Euler , L. Gerhardt , L. Gustafsson , A. Hallgren , J. C. Hanson , M. H. Israel , J. Kiryluk , S. Klein , S. Kleinfelder , A. Nelles , H. Niederhausen , M. A. Olevitch , C. Persichelli , K. Ratzlaff , B. F. Rauch , C. Reed , M. Roumi , A. Samanta , G. E. Simburger , T. Stezelberger , J. Tatar , U. Uggerhoj , J. Walker , R. Young

Design and Expected Performance of the IceCube-Gen2 Surface Array and its Radio Component (ARENA2022)

IceCube-Gen2, the next generation of the IceCube Neutrino Observatory at the South Pole, will consist of three co-located arrays: a deep Optical Array and a more shallow and larger Radio Array for neutrino detection in the ice, and a…

High Energy Astrophysical Phenomena · Physics 2023-06-12 Frank G. Schröder

Livetime and sensitivity of the ARIANNA Hexagonal Radio Array

The ARIANNA collaboration completed the installation of the hexagonal radio array (HRA) in December 2014, serving as a pilot program for a planned high energy neutrino telescope located about 110 km south of McMurdo Station on the Ross Ice…

Instrumentation and Methods for Astrophysics · Physics 2015-09-02 ARIANNA Collaboration , S. W. Barwick , E. C. Berg , D. Z. Besson , G. Binder , W. R. Binns , D. Boersma , R. G. Bose , D. L. Braun , J. H. Buckley , V. Bugaev , S. Buitink , K. Dookayka , P. F. Dowkontt , T. Duffin , S. Euler , L. Gerhardt , L. Gustafsson , A. Hallgren , J. C. Hanson , M. H. Israel , J. Kiryluk , S. Klein , S. Kleinfelder , A. Nelles , H. Niederhausen , M. A. Olevitch , C. Persichelli , K. Ratzlaff , B. F. Rauch , C. Reed , M. Roumi , A. Samanta , G. E. Simburger , T. Stezelberger , J. Tatar , U. Uggerhoj , J. Walker , R. Young

Performance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos

Ultra-high energy neutrinos are interesting messenger particles since, if detected, they can transmit exclusive information about ultra-high energy processes in the Universe. These particles, with energies above $10^{16}\mathrm{eV}$,…

High Energy Astrophysical Phenomena · Physics 2016-10-19 ARA Collaboration , P. Allison , R. Bard , J. J. Beatty , D. Z. Besson , C. Bora , C. -C. Chen , C. -H. Chen , P. Chen , A. Christenson , A. Connolly , J. Davies , M. Duvernois , B. Fox , R. Gaior , P. W. Gorham , K. Hanson , J. Haugen , B. Hill , K. D. Hoffman , E. Hong , S. -Y. Hsu , L. Hu , J. -J. Huang , M. -H. A. Huang , A. Ishihara , A. Karle , J. L. Kelley , D. Kennedy , I. Kravchenko , T. Kuwabara , H. Landsman , A. Laundrie , C. -J. Li , T. C. Liu , M. -Y. Lu , L. Macchiarulo , K. Mase , T. Meures , R. Meyhandan , C. Miki , R. Morse , J. Nam , R. J. Nichol , G. Nir , A. Novikov , A. O'Murchadha , C. Pfendner , K. Ratzlaff , M. Relich , M. Richman , L. Ritter , B. Rotter , P. Sandstrom , P. Schellin , A. Shultz , D. Seckel , Y. -S. Shiao , J. Stockham , M. Stockham , J. Touart , G. S. Varner , M. -Z. Wang , S. -H. Wang , Y. Yang , S. Yoshida , R. Young

IceRay: An IceCube-centered Radio-Cherenkov GZK Neutrino Detector

We discuss design considerations and simulation results for IceRay, a proposed large-scale ultra-high energy (UHE) neutrino detector at the South Pole. The array is designed to detect the coherent Askaryan radio emission from UHE neutrino…

High Energy Astrophysical Phenomena · Physics 2010-04-30 P. Allison , J. Beatty , P. Chen , A. Connolly , M. DuVernois , P. Gorham , F. Halzen , K. Hanson , K. Hoffman , A. Karle , J. L. Kelley , H. Landsman , J. Learned , C. Miki , R. Morse , R. Nichol , C. Rott , L. Ruckman , D. Seckel , G. Varner , D. Williams

Framework and Tools for the Simulation and Analysis of the Radio Emission from Air Showers at IceCube

The Surface Enhancement of the IceTop air-shower array will include the addition of radio antennas and scintillator panels, co-located with the existing ice-Cherenkov tanks and covering an area of about 1 km$^2$. Together, these will…

High Energy Astrophysical Phenomena · Physics 2022-10-25 R. Abbasi , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , J. M. Alameddine , A. A. Alves , N. M. Amin , K. Andeen , T. Anderson , G. Anton , C. Argüelles , Y. Ashida , S. Axani , X. Bai , A. Balagopal V. , S. W. Barwick , B. Bastian , V. Basu , S. Baur , R. Bay , J. J. Beatty , K. -H. Becker , J. Becker Tjus , J. Beise , C. Bellenghi , S. Benda , S. BenZvi , D. Berley , E. Bernardini , D. Z. Besson , G. Binder , D. Bindig , E. Blaufuss , S. Blot , M. Boddenberg , F. Bontempo , J. Y. Book , J. Borowka , S. Böser , O. Botner , J. Böttcher , E. Bourbeau , F. Bradascio , J. Braun , B. Brinson , S. Bron , J. Brostean-Kaiser , R. T. Burley , R. S. Busse , M. A. Campana , E. G. Carnie-Bronca , C. Chen , Z. Chen , D. Chirkin , K. Choi , B. A. Clark , K. Clark , L. Classen , A. Coleman , G. H. Collin , A. Connolly , J. M. Conrad , P. Coppin , P. Correa , D. F. Cowen , R. Cross , C. Dappen , P. Dave , C. De Clercq , J. J. DeLaunay , D. Delgado López , H. Dembinski , K. Deoskar , A. Desai , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , A. Diaz , J. C. Díaz-Vélez , M. Dittmer , H. Dujmovic , M. Dunkman , M. A. DuVernois , T. Ehrhardt , P. Eller , R. Engel , H. Erpenbeck , J. Evans , P. A. Evenson , K. L. Fan , A. R. Fazely , A. Fedynitch , N. Feigl , S. Fiedlschuster , A. T. Fienberg , C. Finley , L. Fischer , D. Fox , A. Franckowiak , E. Friedman , A. Fritz , P. Fürst , T. K. Gaisser , J. Gallagher , E. Ganster , A. Garcia , S. Garrappa , L. Gerhardt , A. Ghadimi , C. Glaser , T. Glauch , T. Glüsenkamp , N. Goehlke , J. G. Gonzalez , S. Goswami , D. Grant , T. Grégoire , S. Griswold , C. Günther , P. Gutjahr , C. Haack , A. Hallgren , R. Halliday , L. Halve , F. Halzen , M. Ha Minh , K. Hanson , J. Hardin , A. A. Harnisch , A. Haungs , D. Hebecker , K. Helbing , F. Henningsen , E. C. Hettinger , S. Hickford , J. Hignight , C. Hill , G. C. Hill , K. D. Hoffman , K. Hoshina , W. Hou , F. Huang , M. Huber , T. Huber , K. Hultqvist , M. Hünnefeld , R. Hussain , K. Hymon , S. In , N. Iovine , A. Ishihara , M. Jansson , G. S. Japaridze , M. Jeong , M. Jin , B. J. P. Jones , D. Kang , W. Kang , X. Kang , A. Kappes , D. Kappesser , L. Kardum , T. Karg , M. Karl , A. Karle , U. Katz , M. Kauer , M. Kellermann , J. L. Kelley , A. Kheirandish , K. Kin , T. Kintscher , J. Kiryluk , S. R. Klein , A. Kochocki , R. Koirala , H. Kolanoski , T. Kontrimas , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , P. Koundal , M. Kovacevich , M. Kowalski , T. Kozynets , E. Krupczak , E. Kun , N. Kurahashi , N. Lad , C. Lagunas Gualda , J. L. Lanfranchi , M. J. Larson , F. Lauber , J. P. Lazar , J. W. Lee , K. Leonard , A. Leszczyńska , Y. Li , M. Lincetto , Q. R. Liu , M. Liubarska , E. Lohfink , C. J. Lozano Mariscal , L. Lu , F. Lucarelli , A. Ludwig , W. Luszczak , Y. Lyu , W. Y. Ma , J. Madsen , K. B. M. Mahn , Y. Makino , S. Mancina , I. C. Mariş , I. Martinez-Soler , R. Maruyama , S. McCarthy , T. McElroy , F. McNally , J. V. Mead , K. Meagher , S. Mechbal , A. Medina , M. Meier , S. Meighen-Berger , J. Micallef , D. Mockler , T. Montaruli , R. W. Moore , R. Morse , M. Moulai , T. Mukherjee , R. Naab , R. Nagai , U. Naumann , J. Necker , L. V. Nguyen , H. Niederhausen , M. U. Nisa , S. C. Nowicki , A. Obertacke Pollmann , M. Oehler , B. Oeyen , A. Olivas , E. O'Sullivan , H. Pandya , D. V. Pankova , N. Park , G. K. Parker , E. N. Paudel , L. Paul , C. Pérez de los Heros , L. Peters , J. Peterson , S. Philippen , S. Pieper , A. Pizzuto , M. Plum , Y. Popovych , A. Porcelli , M. Prado Rodriguez , B. Pries , G. T. Przybylski , C. Raab , J. Rack-Helleis , A. Raissi , M. Rameez , K. Rawlins , I. C. Rea , Z. Rechav , A. Rehman , P. Reichherzer , R. Reimann , G. Renzi , E. Resconi , S. Reusch , W. Rhode , M. Richman , B. Riedel , E. J. Roberts , S. Robertson , G. Roellinghoff , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , D. Rysewyk Cantu , I. Safa , J. Saffer , D. Salazar-Gallegos , P. Sampathkumar , S. E. Sanchez Herrera , A. Sandrock , M. Santander , S. Sarkar , S. Sarkar , K. Satalecka , M. Schaufel , H. Schieler , S. Schindler , T. Schmidt , A. Schneider , J. Schneider , F. G. Schröder , L. Schumacher , G. Schwefer , S. Sclafani , D. Seckel , S. Seunarine , A. Sharma , S. Shefali , N. Shimizu , M. Silva , B. Skrzypek , B. Smithers , R. Snihur , J. Soedingrekso , D. Soldin , C. Spannfellner , G. M. Spiczak , C. Spiering , J. Stachurska , M. Stamatikos , T. Stanev , R. Stein , J. Stettner , T. Stezelberger , T. Stürwald , T. Stuttard , G. W. Sullivan , I. Taboada , S. Ter-Antonyan , J. Thwaites , S. Tilav , F. Tischbein , K. Tollefson , C. Tönnis , S. Toscano , D. Tosi , A. Trettin , M. Tselengidou , C. F. Tung , A. Turcati , R. Turcotte , C. F. Turley , J. P. Twagirayezu , B. Ty , M. A. Unland Elorrieta , N. Valtonen-Mattila , J. Vandenbroucke , N. van Eijndhoven , D. Vannerom , J. van Santen , J. Veitch-Michaelis , S. Verpoest , C. Walck , W. Wang , T. B. Watson , C. Weaver , P. Weigel , A. Weindl , M. J. Weiss , J. Weldert , C. Wendt , J. Werthebach , M. Weyrauch , N. Whitehorn , C. H. Wiebusch , N. Willey , D. R. Williams , M. Wolf , G. Wrede , J. Wulff , X. W. Xu , J. P. Yanez , E. Yildizci , S. Yoshida , S. Yu , T. Yuan , Z. Zhang , P. Zhelnin

Recent results from the ARIANNA neutrino experiment

The ARIANNA experiment is currently taking data in its pilot-phase on the Ross ice-shelf. Fully autonomous stations measure radio signals in the frequency range from 100 MHz to 1 GHz. The seven station HRA was completed in December 2014,…

Instrumentation and Methods for Astrophysics · Physics 2017-04-05 Anna Nelles

Advancing ARA: the Next-Generation (ARA-Next) DAQ System

The Askaryan Radio Array (ARA) has been operating at the South Pole for over a decade, searching for ultra-high energy astrophysical and cosmogenic neutrinos using the Askaryan effect. ARA has consistently served as a testbed for innovative…

Instrumentation and Methods for Astrophysics · Physics 2025-09-24 Pawan Giri

Radio detection of high-energy cosmic rays with the Auger Engineering Radio Array (PISA 2015)

The Auger Engineering Radio Array (AERA) is an enhancement of the Pierre Auger Observatory in Argentina. Covering about View the $17\,$km$^2$, AERA is the world-largest antenna array for cosmic-ray observation. It consists of more than 150…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Frank G. Schröder

IceCube : Toward a km^3 Neutrino Telescope

Since the end of the 2005-2006 austral summer, the IceCube detector consists of an array of 9 strings, deployed between 1450 m and 2450 m of depth and containing 540 digital optical sensors and 16 IceTop surface stations with 64 sensors.…

Astrophysics · Physics 2019-08-14 Paolo Desiati

A radio air shower surface detector as an extension for IceCube and IceTop

The IceCube neutrino detector is built into the Antarctic ice sheet at the South Pole to measure high energy neutrinos. For this, 4800 photomultiplier tubes (PMTs) are being deployed at depths between 1450 and 2450 meters into the ice to…

Astrophysics · Physics 2010-04-30 J. Auffenberg , T. Gaisser , K. Helbing , T. Huege , T. Karg , A. Karle

Physics potential of the IceCube Upgrade for atmospheric neutrino oscillations

The IceCube Upgrade is an extension of the existing IceCube Neutrino Observatory and will be deployed in the 2025-2026 austral summer. It will significantly improve the sensitivity of the detector to atmospheric neutrino oscillations. The…

High Energy Physics - Experiment · Physics 2025-09-17 IceCube Collaboration

High-Fidelity Simulations of the Full Askaryan Radio Array and its Sensitivity to Ultra-High Energy Neutrinos

The Askaryan Radio Array (ARA) is a five-station, in-ice radio detector located at the South Pole searching for particle cascades from cosmogenic and astrophysical neutrinos with $\geq10^{17}$ eV of energy. Cascades in this energy regime…

High Energy Astrophysical Phenomena · Physics 2025-09-23 Abigail Bishop , Alan Salcedo Gomez , Marco Stein Muzio

Updated Results from the RICE Experiment and Future Prospects for Ultra-High Energy Neutrino Detection at the South Pole

The RICE experiment seeks observation of ultra-high energy (UHE; >100 PeV) neutrinos interacting in Antarctic ice, by measurement of the radiowavelength Cherenkov radiation resulting from the collision of a neutrino with an ice molecule.…

High Energy Astrophysical Phenomena · Physics 2013-05-30 Ilya Kravchenko , Dave Seckel , Dave Besson , John Ralston , John Taylor , Ken Ratzlaff , Rob Young

A prototype station for ARIANNA: a detector for cosmic neutrinos

The Antarctic Ross Iceshelf Antenna Neutrino Array (ARIANNA) is a proposed detector for ultra-high energy astrophysical neutrinos. It will detect coherent radio Cherenkov emission from the particle showers produced by neutrinos with…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Lisa Gerhardt , Spencer R. Klein , Thorsten Stezelberger , Steve Barwick , Kamlesh Dookayka , Jordan Hanson , Ryan Nichol