Related papers: Cosmic Ray Detection with the IceTop Enhancement

The IceCube-Gen2 Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)

IceCube-Gen2 is a planned next-generation neutrino observatory at the South Pole that builds upon the successful design of IceCube. Integrating two complementary detection technologies for neutrinos, optical and radio Cherenkov emission, in…

High Energy Astrophysical Phenomena · Physics 2023-07-26 IceCube-Gen2 , : , R. Abbasi , M. Ackermann , J. Adams , S. K. Agarwalla , J. A. Aguilar , M. Ahlers , J. M. Alameddine , N. M. Amin , K. Andeen , G. Anton , C. Argüelles , Y. Ashida , S. Athanasiadou , J. Audehm , S. N. Axani , X. Bai , A. Balagopal V. , M. Baricevic , S. W. Barwick , V. Basu , R. Bay , J. Becker Tjus , J. Beise , C. Bellenghi , C. Benning , S. BenZvi , D. Berley , E. Bernardini , D. Z. Besson , A. Bishop , E. Blaufuss , S. Blot , M. Bohmer , F. Bontempo , J. Y. Book , J. Borowka , C. Boscolo Meneguolo , S. Böser , O. Botner , J. Böttcher , S. Bouma , E. Bourbeau , J. Braun , B. Brinson , J. Brostean-Kaiser , R. T. Burley , R. S. Busse , D. Butterfield , M. A. Campana , K. Carloni , E. G. Carnie-Bronca , M. Cataldo , S. Chattopadhyay , N. Chau , C. Chen , Z. Chen , D. Chirkin , S. Choi , B. A. Clark , R. Clark , L. Classen , A. Coleman , G. H. Collin , J. M. Conrad , D. F. Cowen , B. Dasgupta , P. Dave , C. Deaconu , C. De Clercq , S. De Kockere , J. J. DeLaunay , D. Delgado , S. Deng , K. Deoskar , A. Desai , P. Desiati , K. D. de Vries , G. de Wasseige , T. DeYoung , A. Diaz , J. C. Díaz-Vélez , M. Dittmer , A. Domi , H. Dujmovic , M. A. DuVernois , T. Ehrhardt , P. Eller , E. Ellinger , S. El Mentawi , D. Elsässer , R. Engel , H. Erpenbeck , J. Evans , J. J. Evans , P. A. Evenson , K. L. Fan , K. Fang , K. Farrag , K. Farrag , A. R. Fazely , A. Fedynitch , N. Feigl , S. Fiedlschuster , C. Finley , L. Fischer , B. Flaggs , D. Fox , A. Franckowiak , A. Fritz , T. Fujii , P. Fürst , J. Gallagher , E. Ganster , A. Garcia , L. Gerhardt , R. Gernhaeuser , A. Ghadimi , P. Giri , C. Glaser , T. Glauch , T. Glüsenkamp , N. Goehlke , S. Goswami , D. Grant , S. J. Gray , O. Gries , S. Griffin , S. Griswold , D. Guevel , C. Günther , P. Gutjahr , C. Haack , T. Haji Azim , A. Hallgren , R. Halliday , S. Hallmann , L. Halve , F. Halzen , H. Hamdaoui , M. Ha Minh , K. Hanson , J. Hardin , A. A. Harnisch , P. Hatch , J. Haugen , A. Haungs , D. Heinen , K. Helbing , J. Hellrung , B. Hendricks , F. Henningsen , J. Henrichs , L. Heuermann , N. Heyer , S. Hickford , A. Hidvegi , J. Hignight , C. Hill , G. C. Hill , K. D. Hoffman , B. Hoffmann , K. Holzapfel , S. Hori , K. Hoshina , W. Hou , T. Huber , T. Huege , K. Hughes , K. Hultqvist , M. Hünnefeld , R. Hussain , K. Hymon , S. In , A. Ishihara , M. Jacquart , O. Janik , M. Jansson , G. S. Japaridze , M. Jeong , M. Jin , B. J. P. Jones , O. Kalekin , D. Kang , W. Kang , X. Kang , A. Kappes , D. Kappesser , L. Kardum , T. Karg , M. Karl , A. Karle , T. Katori , U. Katz , M. Kauer , J. L. Kelley , A. Khatee Zathul , A. Kheirandish , J. Kiryluk , S. R. Klein , T. Kobayashi , A. Kochocki , H. Kolanoski , T. Kontrimas , L. Köpke , C. Kopper , D. J. Koskinen , P. Koundal , M. Kovacevich , M. Kowalski , T. Kozynets , C. B. Krauss , I. Kravchenko , J. Krishnamoorthi , E. Krupczak , A. Kumar , E. Kun , N. Kurahashi , N. Lad , C. Lagunas Gualda , M. J. Larson , S. Latseva , F. Lauber , J. P. Lazar , J. W. Lee , K. Leonard DeHolton , A. Leszczyńska , M. Lincetto , Q. R. Liu , M. Liubarska , M. Lohan , E. Lohfink , J. LoSecco , C. Love , C. J. Lozano Mariscal , L. Lu , F. Lucarelli , Y. Lyu , J. Madsen , K. B. M. Mahn , Y. Makino , S. Mancina , S. Mandalia , W. Marie Sainte , I. C. Mariş , S. Marka , Z. Marka , M. Marsee , I. Martinez-Soler , R. Maruyama , F. Mayhew , T. McElroy , F. McNally , J. V. Mead , K. Meagher , S. Mechbal , A. Medina , M. Meier , Y. Merckx , L. Merten , Z. Meyers , J. Micallef , M. Mikhailova , J. Mitchell , T. Montaruli , R. W. Moore , Y. Morii , R. Morse , M. Moulai , T. Mukherjee , R. Naab , R. Nagai , M. Nakos , A. Narayan , U. Naumann , J. Necker , A. Negi , A. Nelles , M. Neumann , H. Niederhausen , M. U. Nisa , A. Noell , A. Novikov , S. C. Nowicki , A. Nozdrina , E. Oberla , A. Obertacke Pollmann , V. O'Dell , M. Oehler , B. Oeyen , A. Olivas , R. Ørsøe , J. Osborn , E. O'Sullivan , L. Papp , N. Park , G. K. Parker , E. N. Paudel , L. Paul , C. Pérez de los Heros , T. C. Petersen , J. Peterson , S. Philippen , S. Pieper , J. L. Pinfold , A. Pizzuto , I. Plaisier , M. Plum , A. Pontén , Y. Popovych , M. Prado Rodriguez , B. Pries , R. Procter-Murphy , G. T. Przybylski , L. Pyras , J. Rack-Helleis , M. Rameez , K. Rawlins , Z. Rechav , A. Rehman , P. Reichherzer , G. Renzi , E. Resconi , S. Reusch , W. Rhode , B. Riedel , M. Riegel , A. Rifaie , E. J. Roberts , S. Robertson , S. Rodan , G. Roellinghoff , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , I. Safa , J. Saffer , D. Salazar-Gallegos , P. Sampathkumar , S. E. Sanchez Herrera , A. Sandrock , P. Sandstrom , M. Santander , S. Sarkar , S. Sarkar , J. Savelberg , P. Savina , M. Schaufel , H. Schieler , S. Schindler , L. Schlickmann , B. Schlüter , F. Schlüter , N. Schmeisser , T. Schmidt , J. Schneider , F. G. Schröder , L. Schumacher , G. Schwefer , S. Sclafani , D. Seckel , M. Seikh , S. Seunarine , M. H. Shaevitz , R. Shah , A. Sharma , S. Shefali , N. Shimizu , M. Silva , B. Skrzypek , D. Smith , B. Smithers , R. Snihur , J. Soedingrekso , A. Søgaard , D. Soldin , P. Soldin , G. Sommani , D. Southall , C. Spannfellner , G. M. Spiczak , C. Spiering , M. Stamatikos , T. Stanev , T. Stezelberger , J. Stoffels , T. Stürwald , T. Stuttard , G. W. Sullivan , I. Taboada , A. Taketa , H. K. M. Tanaka , S. Ter-Antonyan , M. Thiesmeyer , W. G. Thompson , J. Thwaites , S. Tilav , K. Tollefson , C. Tönnis , J. Torres , S. Toscano , D. Tosi , A. Trettin , Y. Tsunesada , C. F. Tung , R. Turcotte , J. P. Twagirayezu , B. Ty , M. A. Unland Elorrieta , A. K. Upadhyay , K. Upshaw , N. Valtonen-Mattila , J. Vandenbroucke , N. van Eijndhoven , D. Vannerom , J. van Santen , J. Vara , D. Veberic , J. Veitch-Michaelis , M. Venugopal , S. Verpoest , A. Vieregg , A. Vijai , C. Walck , C. Weaver , P. Weigel , A. Weindl , J. Weldert , C. Welling , C. Wendt , J. Werthebach , M. Weyrauch , N. Whitehorn , C. H. Wiebusch , N. Willey , D. R. Williams , S. Wissel , L. Witthaus , A. Wolf , M. Wolf , G. Wörner , G. Wrede , S. Wren , X. W. Xu , J. P. Yanez , E. Yildizci , S. Yoshida , R. Young , F. Yu , S. Yu , T. Yuan , Z. Zhang , P. Zhelnin , S. Zierke , M. Zimmerman

The Surface Array of IceCube-Gen2

The science goals of IceCube-Gen2 include multi-messenger astronomy, astroparticle and particle physics. To this end, the observatory will include several detection methods, including a surface array and in-ice optical sensors. The array…

High Energy Astrophysical Phenomena · Physics 2023-08-08 Alan Coleman

Anisotropy of TeV and PeV cosmic rays with IceCube and IceTop

The interaction of high energy cosmic rays with the Earth's atmosphere produces extensive air showers of secondary particles with a large muon component. By exploiting the sensitivity of neutrino telescopes to high energy muons, it is…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Marcos Santander

Cosmic-Ray Physics at the South Pole

The geographic South Pole provides unique opportunities to study cosmic particles in the Southern Hemisphere. It represents an optimal location to deploy large-scale neutrino telescopes in the deep Antarctic ice, such as AMANDA or IceCube.…

High Energy Astrophysical Phenomena · Physics 2024-05-21 D. Soldin , P. A. Evenson , H. Kolanoski , A. A. Watson

Three-year performance of the IceAct telescopes at the IceCube Neutrino Observatory

IceAct is an array of compact Imaging Air Cherenkov Telescopes at the ice surface as part of the IceCube Neutrino Observatory. The telescopes, featuring a camera of 61 silicon photomultipliers and fresnel-lens-based optics, are optimized to…

High Energy Astrophysical Phenomena · Physics 2025-09-17 Lars Heuermann

Improved Detection of Supernovae with the IceCube Observatory

The IceCube neutrino telescope monitors one cubic kilometer of deep Antarctic ice by detecting Cherenkov photons emitted from charged secondaries produced when neutrinos interact in the ice. The geometry of the detector, which comprises a…

High Energy Astrophysical Phenomena · Physics 2018-07-04 Lutz Köpke

The IceCube Collaboration -- Contributions to the 37th International Cosmic Ray Conference (ICRC2021)

This list of contributions to the 37th International Cosmic Ray Conference in Berlin, Germany (12-23 July 2021) summarizes the latest results from the IceCube Neutrino Observatory. IceCube, completed 10 years ago at the geographic South…

High Energy Astrophysical Phenomena · Physics 2021-07-16 IceCube Collaboration , R. Abbasi , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , C. Alispach , A. A. Alves , N. M. Amin , R. An , K. Andeen , T. Anderson , G. Anton , C. Argüelles , Y. Ashida , S. Axani , X. Bai , A. Balagopal V. , A. Barbano , S. W. Barwick , B. Bastian , V. Basu , S. Baur , R. Bay , J. J. Beatty , K. -H. Becker , J. Becker Tjus , C. Bellenghi , S. BenZvi , D. Berley , E. Bernardini , D. Z. Besson , G. Binder , D. Bindig , E. Blaufuss , S. Blot , M. Boddenberg , F. Bontempo , J. Borowka , S. Böser , O. Botner , J. Böttcher , E. Bourbeau , F. Bradascio , J. Braun , S. Bron , J. Brostean-Kaiser , S. Browne , A. Burgman , R. T. Burley , R. S. Busse , M. A. Campana , E. G. Carnie-Bronca , C. Chen , D. Chirkin , K. Choi , B. A. Clark , K. Clark , L. Classen , A. Coleman , G. H. Collin , J. M. Conrad , P. Coppin , P. Correa , D. F. Cowen , R. Cross , C. Dappen , P. Dave , C. De Clercq , J. J. DeLaunay , H. Dembinski , K. Deoskar , S. De Ridder , A. Desai , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , S. Dharani , A. Diaz , J. C. Díaz-Vélez , M. Dittmer , H. Dujmovic , M. Dunkman , M. A. DuVernois , E. Dvorak , T. Ehrhardt , P. Eller , R. Engel , H. Erpenbeck , J. Evans , P. A. Evenson , K. L. Fan , A. R. Fazely , S. Fiedlschuster , A. T. Fienberg , K. Filimonov , 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 , A. Goldschmidt , J. G. Gonzalez , S. Goswami , D. Grant , T. Grégoire , S. Griswold , M. Gündüz , C. Günther , C. Haack , A. Hallgren , R. Halliday , L. Halve , F. Halzen , M. Ha Minh , K. Hanson , J. Hardin , A. A. Harnisch , A. Haungs , S. Hauser , D. Hebecker , K. Helbing , F. Henningsen , E. C. Hettinger , S. Hickford , J. Hignight , C. Hill , G. C. Hill , K. D. Hoffman , R. Hoffmann , T. Hoinka , B. Hokanson-Fasig , K. Hoshina , F. Huang , M. Huber , T. Huber , K. Hultqvist , M. Hünnefeld , R. Hussain , S. In , N. Iovine , A. Ishihara , M. Jansson , G. S. Japaridze , M. Jeong , B. J. P. Jones , D. Kang , W. Kang , X. Kang , A. Kappes , D. Kappesser , 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 , R. Koirala , H. Kolanoski , T. Kontrimas , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , P. Koundal , M. Kovacevich , M. Kowalski , T. Kozynets , 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 , R. Maruyama , K. Mase , T. McElroy , F. McNally , J. V. Mead , K. Meagher , A. Medina , M. Meier , S. Meighen-Berger , J. Micallef , D. Mockler , T. Montaruli , R. W. Moore , R. Morse , M. Moulai , R. Naab , R. Nagai , U. Naumann , J. Necker , L. V. Nguyên , H. Niederhausen , M. U. Nisa , S. C. Nowicki , D. R. Nygren , A. Obertacke Pollmann , M. Oehler , 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 , D. Pieloth , S. Pieper , M. Pittermann , A. Pizzuto , M. Plum , Y. Popovych , A. Porcelli , M. Prado Rodriguez , P. B. Price , B. Pries , G. T. Przybylski , C. Raab , A. Raissi , M. Rameez , K. Rawlins , I. C. Rea , 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 , S. E. Sanchez Herrera , A. Sandrock , J. Sandroos , M. Santander , S. Sarkar , S. Sarkar , K. Satalecka , M. Scharf , M. Schaufel , H. Schieler , S. Schindler , P. Schlunder , T. Schmidt , A. Schneider , J. Schneider , F. G. Schröder , L. Schumacher , G. Schwefer , S. Sclafani , D. Seckel , S. Seunarine , A. Sharma , S. Shefali , 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 , A. Steuer , T. Stezelberger , T. Stürwald , T. Stuttard , G. W. Sullivan , I. Taboada , F. Tenholt , S. Ter-Antonyan , S. Tilav , F. Tischbein , K. Tollefson , L. Tomankova , 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 , S. Verpoest , M. Vraeghe , C. Walck , 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 , D. R. Williams , M. Wolf , K. Woschnagg , G. Wrede , J. Wulff , X. W. Xu , Y. Xu , J. P. Yanez , S. Yoshida , S. Yu , T. Yuan , Z. Zhang

IceCube as a discovery observatory for physics beyond the standard model

Construction of the cubic-kilometer neutrino detector IceCube at the South Pole has been completed in December 2010. It forms a lattice of 5160 photomultiplier tubes monitoring a gigaton of the deep Antarctic ice for particle induced…

High Energy Physics - Experiment · Physics 2019-08-13 K. Helbing

Physics Capabilities of the IceCube DeepCore Detector

IceCube-DeepCore is a compact Cherenkov detector located in the clear ice of the bottom center of the IceCube Neutrino Telescope. Its purpose is to enhance the sensitivity of IceCube for low neutrino energies (< 1 TeV) and to lower the…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Christopher Wiebusch

Improved Gamma-Hadron Separation for PeV Photon Searches with IceCube (ICRC 2025)

IceTop, the km$^2$ surface array of the IceCube Neutrino Observatory at the South Pole, is sensitive to air showers of all primary particles, including gamma rays. In particular, in the PeV energy range, the combination of IceTop and…

High Energy Astrophysical Phenomena · Physics 2025-07-09 Frank G. Schröder , Federico Bontempo

Mastering 3D-detection of Extensive Air Showers in Cherenkov Light

A new SPHERE seires complex extensive air showers detector is under development. The main goal of its mission is to study the mass composition of cosmic ray nuclei in the 1-100 PeV energy range at a new level. The already well-established…

High Energy Astrophysical Phenomena · Physics 2025-10-16 Elena A. Bonvech , Olga V. Cherkesova , Dmitriy V. Chernov , Elena L. Entina , Vladimir I. Galkin , Vladimir A. Ivanov , Timofey A. Kolodkin , Natalia O. Ovcharenko , Dmitriy A. Podgrudkov , Tatiana M. Roganova , Maxim D. Ziva

Results from IceCube

The IceCube Neutrino Observatory is the world's largest neutrino detector, instrumenting a cubic kilometer of ice at the geographic South Pole. The detector probes neutrino energies from GeV to PeV, and collects high statistics neutrino…

High Energy Astrophysical Phenomena · Physics 2019-09-12 Dawn R. Williams

First Results from IceCube

IceCube is a 1 km$^3$ neutrino observatory being built to study neutrino production in active galactic nuclei, gamma-ray bursts, supernova remnants, and a host of other astrophysical sources. High-energy neutrinos may signal the sources of…

Astrophysics · Physics 2019-08-14 Spencer R. Klein

Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics

The IceCube Observatory is a km^3 neutrino telescope currently under construction at the geographic South Pole. It will comprise 4800 optical sensors deployed on 80 vertical strings between 1450 and 2450 meters under the ice surface.…

Astrophysics · Physics 2019-08-13 Paolo Desiati

Science Potential and Technical Design of the IceCube-Gen2 Surface Array (UHECR 2024)

IceCube-Gen2, the next generation extension of the IceCube Neutrino Observatory at the South Pole, offers a unique scientific potential for cosmic-ray physics at PeV to EeV energies complementing the main science case of neutrino astronomy.…

High Energy Astrophysical Phenomena · Physics 2025-02-28 Frank G. Schroeder

Observation of the anisotropy in arrival direction of Cosmic Rays with IceCube

The IceCube Neutrino Observatory is a kilometer-scale detector currently under construction at the South Pole. In its final configuration the detector will comprise 5160 Digital Optical Modules (DOMs) deployed on 86 strings between 1.5-2.5…

High Energy Astrophysical Phenomena · Physics 2019-08-21 S. Toscano

IceCube - the next generation neutrino telescope at the South Pole

IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near the South Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos,…

Astrophysics · Physics 2019-08-14 A. Karle

Spectrum of PeV Cosmic-Ray Protons and Helium Nuclei with IceCube

The IceCube Observatory comprises a cubic-kilometer particle detector deep in the Antarctic ice and the cosmic-ray air-shower array IceTop at the surface above. Previous analyses of the cosmic-ray composition have used coincident events…

High Energy Astrophysical Phenomena · Physics 2025-11-10 Julian Saffer

Is the Ultra-High Energy Cosmic-Ray Excess Observed by the Telescope Array Correlated with IceCube Neutrinos?

The Telescope Array (TA) has observed a statistically significant excess in cosmic-rays with energies above 57 EeV in a region of approximately 1150 square degrees centered on coordinates (R.A. = 146.7, Dec. = 43.2). We note that the…

High Energy Astrophysical Phenomena · Physics 2016-07-05 Ke Fang , Toshihiro Fujii , Tim Linden , Angela V. Olinto

Cosmic Ray Physics with the IceCube Observatory

The IceCube Neutrino Observatory with its 1-km^3 in-ice detector and the 1-km^2 surface detector (IceTop) constitutes a three-dimensional cosmic ray detector well suited for general cosmic ray physics. Various measurements of cosmic ray…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Hermann Kolanoski