Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube

Aartsen MG, Ackermann M, Adams J, Aguilar JA, Ahlers M, Ahrens M, Alispach C, Andeen K, Anderson T, Ansseau , Anton G, Arguelles C, Auffenberg J, Axani S, Backes P, Bagherpour H, Bai X, Barbano A, Barwick SW, Baum , Baur S, Bay R, Beatty JJ, Becker KH, Tjus JB, Benzvi S, Berley D, Bernardini E, Besson DZ, Binder G, Bindig D, Blaufuss E, Blot S, Bohm C, Boerner M, Boeser S, Botner O, Boettcher J, Bourbeau E, Bourbeau J, Bradascio F, Braun J, Bretz HP, Bron S, Brostean-Kaiser J, Burgman A, Buscher J, Busse RS, Carver T, Chen C, Cheung E, Chirkin D, Clark K, Classen L, Collin GH, Conrad JM, Coppin P, Correa P, Cowen DF, Cross R, Dave P, De Andre JPAM, De Clercq C, Delaunay JJ, Dembinski H, Deoskar K, De Ridder S, Desiati P, De Vries KD, De Wasseige G, De With M, Deyoung T, Diaz A, Diaz-Velez JC, Dujmovic H, Dunkman M, Dvorak E, Eberhardt B, Ehrhardt T, Eller P, Evenson PA, Fahey S, Fazely AR, Felde J, Feusels T, Filimonov K, Finley C, Franckowiak A, Friedman E, Fritz A, Gaisser TK, Gallagher J, Ganster E, Garrappa S, Gerhardt L, Ghorbani K, Glauch T, Glüsenkamp T, Goldschmidt A, Gonzalez JG, Grant D, Griffith Z, Guender M, Guenduez M, Haack C, Hallgren A, Halve L, Halzen F, Hanson K, Hebecker D, Heereman D, Heix P, Helbing K, Hellauer R, Henningsen F, Hickford S, Hignight J, Hill GC, Hoffman KD, Hoffmann R, Hoinka T, Hokanson-Fasig B, Hoshina K, Huang F, Huber M, Hultqvist K, Huennefeld M, Hussain R, In S, Iovine N, Ishihara A, Jacobi E, Japaridze GS, Jeong M, Jero K, Jones BJP, Jonske F, Joppe R, Kang W, Kappes A, Kappesser D, Karg T, Karl M, Karle A, Katz U, Kauer M, Kelley JL, Kheirandish A, Kim J, Kintscher T, Kiryluk J, Kittler T, Klein SR, Koirala R, Kolanoski H, Koepke L, Kopper C, Kopper S, Koskinen DJ, Kowalski M, Krings K, Krueckl G, Kulacz N, Kunwar S, Kurahashi N, Kyriacou A, Labare M, Lanfranchi JL, Larson MJ, Lauber F, Lazar JP, Leonard K, Leuermann M, Liu QR, Lohfink E, Mariscal CJL, Lu L, Lucarelli F, Lunemann J, Luszczak W, Madsen J, Maggi G, Mahn KBM, Makino Y, Mallik P, Mallot K, Mancina S, Mari IC, Maruyama R, Mase K, Maunu R, Meagher K, Medici M, Medina A, Meier M, Meighen-Berger S, Menne T, Merino G, Meures T, Miarecki S, Micallef J, Momente G, Montaruli T, Moore RW, Morse R, Moulai M, Muth P, Nagai R, Nahnhauer R, Nakarmi P, Naumann U, Neer G, Niederhausen H, Nowicki SC, Nygren DR, Pollmann AO, Olivas A, O'Murchadha A, O'Sullivan E, Palczewski T, Pandya H, Pankova D, Park N, Peiffer P, De Los Heros CP, Philippen S, Pieloth D, Pinat E, Pizzuto A, Plum M, Porcelli A, Price PB, Przybylski GT, Raab C, Raissi A, Rameez M, Rauch L, Rawlins K, Rea IC, Reimann R, Relethford B, Renzi G, Resconi E, Rhode W, Richman M, Robertson S, Rongen M, Rott C, Ruhe T, Ryckbosch D, Rysewyk D, Safa , Herrera SES, Sandrock A, Sandroos J, Santander M, Sarkar S, Satalecka K, Schaufel M, Schlunder P, Schmidt T, Schneider A, Schneider J, Schumacher L, Sclafani S, Seckel D, Seunarine S, Shefali S, Silva M, Snihur R, Soedingrekso J, Soldin D, Song M, Spiczak GM, Spiering C, Stachurska J, Stamatikos M, Stanev T, Stasik A, Stein R, Stettner J, Steuer A, Stezelberger T, Stokstad RG, Stossl A, Strotjohann NL, Stuerwald T, Stuttard T, Sullivan GW, Sutherland M, Taboada , Tenholt F, Ter-Antonyan S, Terliuk A, Tilav S, Tomankova L, Tonnis C, Toscano S, Tosi D, Tselengidou M, Tung CF, Turcati A, Turcotte R, Turley CF, Ty B, Unger E, Elorrieta MAU, Usner M, Vandenbroucke J, Van Driessche W, Van Eijk D, Van Eijndhoven N, Vanheule S, Van Santen J, Vraeghe M, Walck C, Wallace A, Wallraff M, Wandkowsky N, Watson TB, Weaver C, Weiss MJ, Weldert J, Wendt C, Werthebach J, Westerhoff S, Whelan BJ, Whitehorn N, Wiebe K, Wiebusch CH, Wille L, Williams DR, Wills L, Wolf M, Wood J, Wood TR, Woschnagg K, Wrede G, Xu DL, Xu XW, Xu Y, Yanez JP, Yodh G, Yoshida S, Yuan T, Zoecklein M (2019)


Publication Type: Journal article

Publication year: 2019

Journal

Book Volume: 100

Journal Issue: 8

DOI: 10.1103/PhysRevD.100.082002

Abstract

We report on measurements of the all-particle cosmic ray energy spectrum and composition in the PeV to EeV energy range using 3 years of data from the IceCube Neutrino Observatory. The IceTop detector measures cosmic ray induced air showers on the surface of the ice, from which the energy spectrum of cosmic rays is determined by making additional assumptions about the mass composition. A separate measurement is performed when IceTop data are analyzed in coincidence with the high-energy muon energy loss information from the deep in-ice IceCube detector. In this measurement, both the spectrum and the mass composition of the primary cosmic rays are simultaneously reconstructed using a neural network trained on observables from both detectors. The performance and relative advantages of these two distinct analyses are discussed, including the systematic uncertainties and the dependence on the hadronic interaction models, and both all-particle spectra as well as individual spectra for elemental groups are presented.

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How to cite

APA:

Aartsen, M.G., Ackermann, M., Adams, J., Aguilar, J.A., Ahlers, M., Ahrens, M.,... Zoecklein, M. (2019). Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube. Physical Review D, 100(8). https://doi.org/10.1103/PhysRevD.100.082002

MLA:

Aartsen, M. G., et al. "Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube." Physical Review D 100.8 (2019).

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