Cosmic Ray Spectrum From 250 Tev To 10 Pev Using Icetop

M. G. Aartsen,R. Abbasi,M. Ackermann,J. Adams,J. A. Aguilar,M. Ahlers,M. Ahrens,C. Alispach,N. M. Amin,K. Andeen,T. Anderson,I. Ansseau,G. Anton,C. Argüelles,J. Auffenberg,S. Axani,H. Bagherpour,X. Bai,A. Barbano,S. W. Barwick,B. Bastian,V. Baum,S. Baur,R. Bay,J. J. Beatty,K.-H. Becker,J. Becker Tjus,S. BenZvi,D. Berley,E. Bernardini,D. Z. Besson,G. Binder,D. Bindig,E. Blaufuss,S. Blot,C. Bohm,S. Böser,O. Botner,J. Böttcher,E. Bourbeau,J. Bourbeau,F. Bradascio,J. Braun,S. Bron,J. Brostean-Kaiser,A. Burgman,J. Buscher,R. S. Busse,T. Carver,C. Chen,E. Cheung,D. Chirkin,S. 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,P. Dave,C. De Clercq,J. J. DeLaunay,H. Dembinski,K. Deoskar,S. De Ridder,P. Desiati,K. D. de Vries,G. de Wasseige,T. DeYoung,S. Dharani,A. Diaz,J. C. Díaz-Vélez,H. Dujmovic,E. Dvorak,B. Eberhardt,T. Ehrhardt,P. Eller,R. Engel,P. A. Evenson,S. Fahey,A. R. Fazely,J. Felde,A. T. Fienberg,K. Filimonov,C. Finley,D. Fox,A. Franckowiak,E. Friedman,A. Fritz,T. K. Gaisser,J. Gallagher,E. Ganster,S. Garrappa,L. Gerhardt,K. Ghorbani,T. Glauch,T. Glüsenkamp,A. Goldschmidt,J. G. Gonzalez,D. Grant,T. Grégoire,Z. Griffith,S. Griswold,M. Günder,M. Gündüz,C. Haack,A. Hallgren,R. Halliday,L. Halve,F. Halzen,K. Hanson,A. Haungs,S. Hauser,D. Hebecker,D. Heereman,P. Heix,K. Helbing,R. Hellauer,F. Henningsen,S. Hickford,J. Hignight,C. Hill,G. C. Hill,K. D. Hoffman,R. Hoffmann,T. Hoinka,B. Hokanson-Fasig,K. Hoshina,M. Huber,T. Huber,K. Hultqvist,M. Hünnefeld,R. Hussain,S. In,N. Iovine,A. Ishihara,M. Jansson,G. S. Japaridze,M. Jeong,K. Jero,B. J. P. Jones,F. Jonske,R. Joppe,D. Kang,W. Kang,A. Kappes,D. Kappesser,T. Karg,M. Karl,A. Karle,U. Katz,M. Kauer,M. Kellermann,J. L. Kelley,A. Kheirandish,J. Kim,T. Kintscher,J. Kiryluk,T. Kittler,S. R. Klein,R. Koirala,H. Kolanoski,L. Köpke,C. Kopper,S. Kopper,D. J. Koskinen,P. Koundal,M. Kowalski,K. Krings,G. Krückl,N. Kulacz,N. Kurahashi,A. Kyriacou,J. L. Lanfranchi,M. J. Larson,F. Lauber,J. P. Lazar,K. Leonard,A. Leszczyńska,Y. Li,Q. R. Liu,E. Lohfink,C. J. Lozano Mariscal,L. Lu,F. Lucarelli,A. Ludwig,J. Lünemann,W. Luszczak,Y. Lyu,W. Y. Ma,J. Madsen,G. Maggi,K. B. M. Mahn,P. Mallik,K. Mallot,S. Mancina,I. C. Mariş,R. Maruyama,K. Mase,R. Maunu,F. McNally,K. Meagher,M. Medici,A. Medina,M. Meier,S. Meighen-Berger,G. Merino,J. Merz,T. Meures,J. Micallef,D. Mockler,G. Momenté,T. Montaruli,R. W. Moore,R. Morse,M. Moulai,P. Muth,R. Nagai,U. Naumann,G. Neer,L. V. Nguyễn,H. Niederhausen,M. U. Nisa,S. C. Nowicki,D. R. Nygren,A. Obertacke Pollmann,M. Oehler,A. Olivas,A. O’Murchadha,E. O’Sullivan,H. Pandya,D. V. Pankova,N. Park,G. K. Parker,E. N. Paudel,P. Peiffer,C. Pérez de los Heros,S. Philippen,D. Pieloth,S. Pieper,E. Pinat,A. Pizzuto,M. Plum,Y. Popovych,A. Porcelli,P. B. Price,G. T. Przybylski,C. Raab,A. Raissi,M. Rameez,L. Rauch,K. Rawlins,I. C. Rea,A. Rehman,R. Reimann,B. Relethford,M. Renschler,G. Renzi,E. Resconi,W. Rhode,M. Richman,S. Robertson,M. Rongen,C. Rott,T. Ruhe,D. Ryckbosch,D. Rysewyk Cantu,I. Safa,S. E. Sanchez Herrera,A. Sandrock,J. Sandroos,M. Santander,S. Sarkar,K. Satalecka,M. Scharf,M. Schaufel,H. Schieler,P. Schlunder,T. Schmidt,A. Schneider,J. Schneider,F. G. Schröder,L. Schumacher,S. Sclafani,D. Seckel,S. Seunarine,S. Shefali,M. Silva,B. Smithers,R. Snihur,J. Soedingrekso,D. Soldin,M. Song,G. M. Spiczak,C. Spiering,J. Stachurska,M. Stamatikos,T. Stanev,R. Stein,J. Stettner,A. Steuer,T. Stezelberger,R. G. Stokstad,N. L. Strotjohann,T. Stürwald,T. Stuttard,G. W. Sullivan,I. Taboada,F. Tenholt,S. Ter-Antonyan,A. Terliuk,S. Tilav,K. Tollefson,L. Tomankova,C. Tönnis,S. Toscano,D. Tosi,A. Trettin,M. Tselengidou,C. F. Tung,A. Turcati,R. Turcotte,C. F. Turley,B. Ty,E. Unger,M. A. Unland Elorrieta,M. Usner,J. Vandenbroucke,W. Van Driessche,D. van Eijk,N. van Eijndhoven,D. Vannerom,J. van Santen,S. Verpoest,M. Vraeghe,C. Walck,A. Wallace,M. Wallraff,N. Wandkowsky,T. B. Watson,C. Weaver,A. Weindl,J. Weldert,C. Wendt,J. Werthebach,B. J. Whelan,N. Whitehorn,K. Wiebe,C. H. Wiebusch,L. Wille,D. R. Williams,L. Wills,M. Wolf,J. Wood,T. R. Wood,K. Woschnagg,G. Wrede,J. Wulff,D. L. Xu,X. W. Xu,Y. Xu,J. P. Yanez,G. Yodh,S. Yoshida,T. Yuan,Z. Zhang,M. Zöcklein

PHYSICAL REVIEW D(2020)

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Abstract
We report here an extension of the measurement of the all-particle cosmic-ray spectrum with IceTop to lower energy. The new measurement gives full coverage of the knee region of the spectrum and reduces the gap in energy between previous IceTop and direct measurements. With a new trigger that selects events in closely spaced detectors in the center of the array, the IceTop energy threshold is lowered by almost an order of magnitude below its previous threshold of 2 PeV. In this paper we explain how the new trigger is implemented, and we describe the new machine-learning method developed to deal with events with very few detectors hit. We compare the results with previous measurements by IceTop and others that overlap at higher energy and with HAWC and Tibet in the 100 TeV range.
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Key words
cosmic ray spectrum,pev
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