All-particle cosmic ray energy spectrum measured with 26 IceTop stations

We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, cor...

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Main Authors: Collaboration, I, Abbasi, R, Abdou, Y, Abu-Zayyad, T, Ackermann, M, Adams, J, Aguilar, J, Ahlers, M, Altmann, D, Andeen, K, Auffenberg, J, Bai, X, Baker, M, Barwick, S, Baum, V, Bay, R, Alba, J, Beattie, K, Beatty, J, Bechet, S, Becker, J, Becker, K, Bell, M, Benabderrahmane, M, BenZvi, S, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, D, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, D, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Brown, A, Buitink, S, Caballero-Mora, K, Carson, M, Casier, M, Chirkin, D, Christy, B, Clevermann, F, Cohen, S, Cowen, D, Silva, A, D'Agostino, M, Danninger, M, Daughhetee, J, Davis, J, Clercq, C, Degner, T, Descamps, F, Desiati, P, Vries-Uiterweerd, G, DeYoung, T, Díaz-Vélez, J, Dreyer, J, Dumm, J, Dunkman, M, Eisch, J, Ellsworth, R, Engdegård, O, Euler, S, Evenson, P, Fadiran, O, Fazely, A, Fedynitch, A, Feintzeig, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Franke, R, Gaisser, T, Gallagher, J, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Goodman, J, Góra, D, Grant, D, Groß, A, Grullon, S, Gurtner, M, Ha, C, Ismail, A, Hallgren, A, Halzen, F, Han, K, Hanson, K, Heimann, P, Heinen, D, Helbing, K, Hellauer, R, Hickford, S, Hill, G, Hoffman, K, Hoffmann, B, Homeier, A, Hoshina, K, Huelsnitz, W, Hulth, P, Hultqvist, K, Hussain, S, Ishihara, A, Jacobi, E, Jacobsen, J, Japaridze, G, Johansson, H, Kappes, A, Karg, T, Karle, A, Kiryluk, J, Kislat, F, Klein, SR, Klepser, S, Köhne, J, Kohnen, G, Kolanoski, H, Köpke, L, Kopper, S, Koskinen, D, Kowalski, M, Krasberg, M, Kroll, G, Kunnen, J, Kurahashi, N, Kuwabara, T, Labare, M, Laihem, K, Landsman, H, Larson, M, Lauer, R, Lünemann, J, Madsen, J, Maruyama, R, Mase, K, Matis, H, Meagher, K, Merck, M, Mészáros, P, Meures, T, Miarecki, S, Middell, E, Milke, N, Miller, J, Montaruli, T, Morse, R, Movit, S, Nahnhauer, R, Nam, J, Naumann, U, Nowicki, S, Nygren, DR, Odrowski, S, Olivas, A, Olivo, M, O'Murchadha, A, Panknin, S, Paul, L, Heros, C, Pieloth, D, Posselt, J, Price, P, Przybylski, G, Rawlins, K, Redl, P, Resconi, E, Rhode, W, Ribordy, M, Richman, M, Riedel, B, Rodrigues, J, Rothmaier, F, Rott, C, Ruhe, T, Rutledge, D, Ruzybayev, B, Ryckbosch, D, Sander, H, Santander, M, Sarkar, S, Schatto, K, Scheel, M, Schmidt, T, Schöneberg, S, Schönwald, A, Schukraft, A, Schulte, L, Schultes, A, Schulz, O, Schunck, M, Seckel, D, Semburg, B, Seo, S, Sestayo, Y, Seunarine, S, Silvestri, A, Smith, M, Spiczak, G, Spiering, C, Stamatikos, M, Stanev, T, Stezelberger, T, Stokstad, R, Stößl, A, Strahler, E, Ström, R, Stüer, M, Sullivan, G, Taavola, H, Taboada, I, Tamburro, A, Ter-Antonyan, S, Tilav, S, Toale, P, Toscano, S, Tosi, D, Eijndhoven, N, Overloop, A, Santen, J, Vehring, M, Voge, M, Walck, C, Waldenmaier, T, Wallraff, M, Walter, M, Wasserman, R, Weaver, C, Wendt, C, Westerhoff, S, Whitehorn, N, Wiebe, K, Wiebusch, C, Williams, DR, Wischnewski, R, Wissing, H, Wolf, M, Wood, T, Woschnagg, K, Xu, C, Xu, D, Xu, X, Yanez, J, Yodh, G, Yoshida, S, Zarzhitsky, P, Zoll, M
Format: Journal article
Language:English
Published: 2012
_version_ 1797085879502635008
author Collaboration, I
Abbasi, R
Abdou, Y
Abu-Zayyad, T
Ackermann, M
Adams, J
Aguilar, J
Ahlers, M
Altmann, D
Andeen, K
Auffenberg, J
Bai, X
Baker, M
Barwick, S
Baum, V
Bay, R
Alba, J
Beattie, K
Beatty, J
Bechet, S
Becker, J
Becker, K
Bell, M
Benabderrahmane, M
BenZvi, S
Berdermann, J
Berghaus, P
Berley, D
Bernardini, E
Bertrand, D
Besson, D
Bindig, D
Bissok, M
Blaufuss, E
Blumenthal, J
Boersma, D
Bohm, C
Bose, D
Böser, S
Botner, O
Brayeur, L
Brown, A
Buitink, S
Caballero-Mora, K
Carson, M
Casier, M
Chirkin, D
Christy, B
Clevermann, F
Cohen, S
Cowen, D
Silva, A
D'Agostino, M
Danninger, M
Daughhetee, J
Davis, J
Clercq, C
Degner, T
Descamps, F
Desiati, P
Vries-Uiterweerd, G
DeYoung, T
Díaz-Vélez, J
Dreyer, J
Dumm, J
Dunkman, M
Eisch, J
Ellsworth, R
Engdegård, O
Euler, S
Evenson, P
Fadiran, O
Fazely, A
Fedynitch, A
Feintzeig, J
Feusels, T
Filimonov, K
Finley, C
Fischer-Wasels, T
Flis, S
Franckowiak, A
Franke, R
Gaisser, T
Gallagher, J
Gerhardt, L
Gladstone, L
Glüsenkamp, T
Goldschmidt, A
Goodman, J
Góra, D
Grant, D
Groß, A
Grullon, S
Gurtner, M
Ha, C
Ismail, A
Hallgren, A
Halzen, F
Han, K
Hanson, K
Heimann, P
Heinen, D
Helbing, K
Hellauer, R
Hickford, S
Hill, G
Hoffman, K
Hoffmann, B
Homeier, A
Hoshina, K
Huelsnitz, W
Hulth, P
Hultqvist, K
Hussain, S
Ishihara, A
Jacobi, E
Jacobsen, J
Japaridze, G
Johansson, H
Kappes, A
Karg, T
Karle, A
Kiryluk, J
Kislat, F
Klein, SR
Klepser, S
Köhne, J
Kohnen, G
Kolanoski, H
Köpke, L
Kopper, S
Koskinen, D
Kowalski, M
Krasberg, M
Kroll, G
Kunnen, J
Kurahashi, N
Kuwabara, T
Labare, M
Laihem, K
Landsman, H
Larson, M
Lauer, R
Lünemann, J
Madsen, J
Maruyama, R
Mase, K
Matis, H
Meagher, K
Merck, M
Mészáros, P
Meures, T
Miarecki, S
Middell, E
Milke, N
Miller, J
Montaruli, T
Morse, R
Movit, S
Nahnhauer, R
Nam, J
Naumann, U
Nowicki, S
Nygren, DR
Odrowski, S
Olivas, A
Olivo, M
O'Murchadha, A
Panknin, S
Paul, L
Heros, C
Pieloth, D
Posselt, J
Price, P
Przybylski, G
Rawlins, K
Redl, P
Resconi, E
Rhode, W
Ribordy, M
Richman, M
Riedel, B
Rodrigues, J
Rothmaier, F
Rott, C
Ruhe, T
Rutledge, D
Ruzybayev, B
Ryckbosch, D
Sander, H
Santander, M
Sarkar, S
Schatto, K
Scheel, M
Schmidt, T
Schöneberg, S
Schönwald, A
Schukraft, A
Schulte, L
Schultes, A
Schulz, O
Schunck, M
Seckel, D
Semburg, B
Seo, S
Sestayo, Y
Seunarine, S
Silvestri, A
Smith, M
Spiczak, G
Spiering, C
Stamatikos, M
Stanev, T
Stezelberger, T
Stokstad, R
Stößl, A
Strahler, E
Ström, R
Stüer, M
Sullivan, G
Taavola, H
Taboada, I
Tamburro, A
Ter-Antonyan, S
Tilav, S
Toale, P
Toscano, S
Tosi, D
Eijndhoven, N
Overloop, A
Santen, J
Vehring, M
Voge, M
Walck, C
Waldenmaier, T
Wallraff, M
Walter, M
Wasserman, R
Weaver, C
Wendt, C
Westerhoff, S
Whitehorn, N
Wiebe, K
Wiebusch, C
Williams, DR
Wischnewski, R
Wissing, H
Wolf, M
Wood, T
Woschnagg, K
Xu, C
Xu, D
Xu, X
Yanez, J
Yodh, G
Yoshida, S
Zarzhitsky, P
Zoll, M
author_facet Collaboration, I
Abbasi, R
Abdou, Y
Abu-Zayyad, T
Ackermann, M
Adams, J
Aguilar, J
Ahlers, M
Altmann, D
Andeen, K
Auffenberg, J
Bai, X
Baker, M
Barwick, S
Baum, V
Bay, R
Alba, J
Beattie, K
Beatty, J
Bechet, S
Becker, J
Becker, K
Bell, M
Benabderrahmane, M
BenZvi, S
Berdermann, J
Berghaus, P
Berley, D
Bernardini, E
Bertrand, D
Besson, D
Bindig, D
Bissok, M
Blaufuss, E
Blumenthal, J
Boersma, D
Bohm, C
Bose, D
Böser, S
Botner, O
Brayeur, L
Brown, A
Buitink, S
Caballero-Mora, K
Carson, M
Casier, M
Chirkin, D
Christy, B
Clevermann, F
Cohen, S
Cowen, D
Silva, A
D'Agostino, M
Danninger, M
Daughhetee, J
Davis, J
Clercq, C
Degner, T
Descamps, F
Desiati, P
Vries-Uiterweerd, G
DeYoung, T
Díaz-Vélez, J
Dreyer, J
Dumm, J
Dunkman, M
Eisch, J
Ellsworth, R
Engdegård, O
Euler, S
Evenson, P
Fadiran, O
Fazely, A
Fedynitch, A
Feintzeig, J
Feusels, T
Filimonov, K
Finley, C
Fischer-Wasels, T
Flis, S
Franckowiak, A
Franke, R
Gaisser, T
Gallagher, J
Gerhardt, L
Gladstone, L
Glüsenkamp, T
Goldschmidt, A
Goodman, J
Góra, D
Grant, D
Groß, A
Grullon, S
Gurtner, M
Ha, C
Ismail, A
Hallgren, A
Halzen, F
Han, K
Hanson, K
Heimann, P
Heinen, D
Helbing, K
Hellauer, R
Hickford, S
Hill, G
Hoffman, K
Hoffmann, B
Homeier, A
Hoshina, K
Huelsnitz, W
Hulth, P
Hultqvist, K
Hussain, S
Ishihara, A
Jacobi, E
Jacobsen, J
Japaridze, G
Johansson, H
Kappes, A
Karg, T
Karle, A
Kiryluk, J
Kislat, F
Klein, SR
Klepser, S
Köhne, J
Kohnen, G
Kolanoski, H
Köpke, L
Kopper, S
Koskinen, D
Kowalski, M
Krasberg, M
Kroll, G
Kunnen, J
Kurahashi, N
Kuwabara, T
Labare, M
Laihem, K
Landsman, H
Larson, M
Lauer, R
Lünemann, J
Madsen, J
Maruyama, R
Mase, K
Matis, H
Meagher, K
Merck, M
Mészáros, P
Meures, T
Miarecki, S
Middell, E
Milke, N
Miller, J
Montaruli, T
Morse, R
Movit, S
Nahnhauer, R
Nam, J
Naumann, U
Nowicki, S
Nygren, DR
Odrowski, S
Olivas, A
Olivo, M
O'Murchadha, A
Panknin, S
Paul, L
Heros, C
Pieloth, D
Posselt, J
Price, P
Przybylski, G
Rawlins, K
Redl, P
Resconi, E
Rhode, W
Ribordy, M
Richman, M
Riedel, B
Rodrigues, J
Rothmaier, F
Rott, C
Ruhe, T
Rutledge, D
Ruzybayev, B
Ryckbosch, D
Sander, H
Santander, M
Sarkar, S
Schatto, K
Scheel, M
Schmidt, T
Schöneberg, S
Schönwald, A
Schukraft, A
Schulte, L
Schultes, A
Schulz, O
Schunck, M
Seckel, D
Semburg, B
Seo, S
Sestayo, Y
Seunarine, S
Silvestri, A
Smith, M
Spiczak, G
Spiering, C
Stamatikos, M
Stanev, T
Stezelberger, T
Stokstad, R
Stößl, A
Strahler, E
Ström, R
Stüer, M
Sullivan, G
Taavola, H
Taboada, I
Tamburro, A
Ter-Antonyan, S
Tilav, S
Toale, P
Toscano, S
Tosi, D
Eijndhoven, N
Overloop, A
Santen, J
Vehring, M
Voge, M
Walck, C
Waldenmaier, T
Wallraff, M
Walter, M
Wasserman, R
Weaver, C
Wendt, C
Westerhoff, S
Whitehorn, N
Wiebe, K
Wiebusch, C
Williams, DR
Wischnewski, R
Wissing, H
Wolf, M
Wood, T
Woschnagg, K
Xu, C
Xu, D
Xu, X
Yanez, J
Yodh, G
Yoshida, S
Zarzhitsky, P
Zoll, M
author_sort Collaboration, I
collection OXFORD
description We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenith angle ranges between 0{\deg} and 46{\deg}. Because of the isotropy of cosmic rays in this energy range the spectra from all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under different assumptions on the primary mass composition. Good agreement of spectra in the three zenith angle ranges was found for the assumption of pure proton and a simple two-component model. For zenith angles {\theta} < 30{\deg}, where the mass dependence is smallest, the knee in the cosmic ray energy spectrum was observed between 3.5 and 4.32 PeV, depending on composition assumption. Spectral indices above the knee range from -3.08 to -3.11 depending on primary mass composition assumption. Moreover, an indication of a flattening of the spectrum above 22 PeV were observed.
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spelling oxford-uuid:a1a72d22-993f-4d87-a55f-dd9098d38ce42022-03-27T02:15:36ZAll-particle cosmic ray energy spectrum measured with 26 IceTop stationsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:a1a72d22-993f-4d87-a55f-dd9098d38ce4EnglishSymplectic Elements at Oxford2012Collaboration, IAbbasi, RAbdou, YAbu-Zayyad, TAckermann, MAdams, JAguilar, JAhlers, MAltmann, DAndeen, KAuffenberg, JBai, XBaker, MBarwick, SBaum, VBay, RAlba, JBeattie, KBeatty, JBechet, SBecker, JBecker, KBell, MBenabderrahmane, MBenZvi, SBerdermann, JBerghaus, PBerley, DBernardini, EBertrand, DBesson, DBindig, DBissok, MBlaufuss, EBlumenthal, JBoersma, DBohm, CBose, DBöser, SBotner, OBrayeur, LBrown, ABuitink, SCaballero-Mora, KCarson, MCasier, MChirkin, DChristy, BClevermann, FCohen, SCowen, DSilva, AD'Agostino, MDanninger, MDaughhetee, JDavis, JClercq, CDegner, TDescamps, FDesiati, PVries-Uiterweerd, GDeYoung, TDíaz-Vélez, JDreyer, JDumm, JDunkman, MEisch, JEllsworth, REngdegård, OEuler, SEvenson, PFadiran, OFazely, AFedynitch, AFeintzeig, JFeusels, TFilimonov, KFinley, CFischer-Wasels, TFlis, SFranckowiak, AFranke, RGaisser, TGallagher, JGerhardt, LGladstone, LGlüsenkamp, TGoldschmidt, AGoodman, JGóra, DGrant, DGroß, AGrullon, SGurtner, MHa, CIsmail, AHallgren, AHalzen, FHan, KHanson, KHeimann, PHeinen, DHelbing, KHellauer, RHickford, SHill, GHoffman, KHoffmann, BHomeier, AHoshina, KHuelsnitz, WHulth, PHultqvist, KHussain, SIshihara, AJacobi, EJacobsen, JJaparidze, GJohansson, HKappes, AKarg, TKarle, AKiryluk, JKislat, FKlein, SRKlepser, SKöhne, JKohnen, GKolanoski, HKöpke, LKopper, SKoskinen, DKowalski, MKrasberg, MKroll, GKunnen, JKurahashi, NKuwabara, TLabare, MLaihem, KLandsman, HLarson, MLauer, RLünemann, JMadsen, JMaruyama, RMase, KMatis, HMeagher, KMerck, MMészáros, PMeures, TMiarecki, SMiddell, EMilke, NMiller, JMontaruli, TMorse, RMovit, SNahnhauer, RNam, JNaumann, UNowicki, SNygren, DROdrowski, SOlivas, AOlivo, MO'Murchadha, APanknin, SPaul, LHeros, CPieloth, DPosselt, JPrice, PPrzybylski, GRawlins, KRedl, PResconi, ERhode, WRibordy, MRichman, MRiedel, BRodrigues, JRothmaier, FRott, CRuhe, TRutledge, DRuzybayev, BRyckbosch, DSander, HSantander, MSarkar, SSchatto, KScheel, MSchmidt, TSchöneberg, SSchönwald, ASchukraft, ASchulte, LSchultes, ASchulz, OSchunck, MSeckel, DSemburg, BSeo, SSestayo, YSeunarine, SSilvestri, ASmith, MSpiczak, GSpiering, CStamatikos, MStanev, TStezelberger, TStokstad, RStößl, AStrahler, EStröm, RStüer, MSullivan, GTaavola, HTaboada, ITamburro, ATer-Antonyan, STilav, SToale, PToscano, STosi, DEijndhoven, NOverloop, ASanten, JVehring, MVoge, MWalck, CWaldenmaier, TWallraff, MWalter, MWasserman, RWeaver, CWendt, CWesterhoff, SWhitehorn, NWiebe, KWiebusch, CWilliams, DRWischnewski, RWissing, HWolf, MWood, TWoschnagg, KXu, CXu, DXu, XYanez, JYodh, GYoshida, SZarzhitsky, PZoll, MWe report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenith angle ranges between 0{\deg} and 46{\deg}. Because of the isotropy of cosmic rays in this energy range the spectra from all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under different assumptions on the primary mass composition. Good agreement of spectra in the three zenith angle ranges was found for the assumption of pure proton and a simple two-component model. For zenith angles {\theta} < 30{\deg}, where the mass dependence is smallest, the knee in the cosmic ray energy spectrum was observed between 3.5 and 4.32 PeV, depending on composition assumption. Spectral indices above the knee range from -3.08 to -3.11 depending on primary mass composition assumption. Moreover, an indication of a flattening of the spectrum above 22 PeV were observed.
spellingShingle Collaboration, I
Abbasi, R
Abdou, Y
Abu-Zayyad, T
Ackermann, M
Adams, J
Aguilar, J
Ahlers, M
Altmann, D
Andeen, K
Auffenberg, J
Bai, X
Baker, M
Barwick, S
Baum, V
Bay, R
Alba, J
Beattie, K
Beatty, J
Bechet, S
Becker, J
Becker, K
Bell, M
Benabderrahmane, M
BenZvi, S
Berdermann, J
Berghaus, P
Berley, D
Bernardini, E
Bertrand, D
Besson, D
Bindig, D
Bissok, M
Blaufuss, E
Blumenthal, J
Boersma, D
Bohm, C
Bose, D
Böser, S
Botner, O
Brayeur, L
Brown, A
Buitink, S
Caballero-Mora, K
Carson, M
Casier, M
Chirkin, D
Christy, B
Clevermann, F
Cohen, S
Cowen, D
Silva, A
D'Agostino, M
Danninger, M
Daughhetee, J
Davis, J
Clercq, C
Degner, T
Descamps, F
Desiati, P
Vries-Uiterweerd, G
DeYoung, T
Díaz-Vélez, J
Dreyer, J
Dumm, J
Dunkman, M
Eisch, J
Ellsworth, R
Engdegård, O
Euler, S
Evenson, P
Fadiran, O
Fazely, A
Fedynitch, A
Feintzeig, J
Feusels, T
Filimonov, K
Finley, C
Fischer-Wasels, T
Flis, S
Franckowiak, A
Franke, R
Gaisser, T
Gallagher, J
Gerhardt, L
Gladstone, L
Glüsenkamp, T
Goldschmidt, A
Goodman, J
Góra, D
Grant, D
Groß, A
Grullon, S
Gurtner, M
Ha, C
Ismail, A
Hallgren, A
Halzen, F
Han, K
Hanson, K
Heimann, P
Heinen, D
Helbing, K
Hellauer, R
Hickford, S
Hill, G
Hoffman, K
Hoffmann, B
Homeier, A
Hoshina, K
Huelsnitz, W
Hulth, P
Hultqvist, K
Hussain, S
Ishihara, A
Jacobi, E
Jacobsen, J
Japaridze, G
Johansson, H
Kappes, A
Karg, T
Karle, A
Kiryluk, J
Kislat, F
Klein, SR
Klepser, S
Köhne, J
Kohnen, G
Kolanoski, H
Köpke, L
Kopper, S
Koskinen, D
Kowalski, M
Krasberg, M
Kroll, G
Kunnen, J
Kurahashi, N
Kuwabara, T
Labare, M
Laihem, K
Landsman, H
Larson, M
Lauer, R
Lünemann, J
Madsen, J
Maruyama, R
Mase, K
Matis, H
Meagher, K
Merck, M
Mészáros, P
Meures, T
Miarecki, S
Middell, E
Milke, N
Miller, J
Montaruli, T
Morse, R
Movit, S
Nahnhauer, R
Nam, J
Naumann, U
Nowicki, S
Nygren, DR
Odrowski, S
Olivas, A
Olivo, M
O'Murchadha, A
Panknin, S
Paul, L
Heros, C
Pieloth, D
Posselt, J
Price, P
Przybylski, G
Rawlins, K
Redl, P
Resconi, E
Rhode, W
Ribordy, M
Richman, M
Riedel, B
Rodrigues, J
Rothmaier, F
Rott, C
Ruhe, T
Rutledge, D
Ruzybayev, B
Ryckbosch, D
Sander, H
Santander, M
Sarkar, S
Schatto, K
Scheel, M
Schmidt, T
Schöneberg, S
Schönwald, A
Schukraft, A
Schulte, L
Schultes, A
Schulz, O
Schunck, M
Seckel, D
Semburg, B
Seo, S
Sestayo, Y
Seunarine, S
Silvestri, A
Smith, M
Spiczak, G
Spiering, C
Stamatikos, M
Stanev, T
Stezelberger, T
Stokstad, R
Stößl, A
Strahler, E
Ström, R
Stüer, M
Sullivan, G
Taavola, H
Taboada, I
Tamburro, A
Ter-Antonyan, S
Tilav, S
Toale, P
Toscano, S
Tosi, D
Eijndhoven, N
Overloop, A
Santen, J
Vehring, M
Voge, M
Walck, C
Waldenmaier, T
Wallraff, M
Walter, M
Wasserman, R
Weaver, C
Wendt, C
Westerhoff, S
Whitehorn, N
Wiebe, K
Wiebusch, C
Williams, DR
Wischnewski, R
Wissing, H
Wolf, M
Wood, T
Woschnagg, K
Xu, C
Xu, D
Xu, X
Yanez, J
Yodh, G
Yoshida, S
Zarzhitsky, P
Zoll, M
All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title_full All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title_fullStr All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title_full_unstemmed All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title_short All-particle cosmic ray energy spectrum measured with 26 IceTop stations
title_sort all particle cosmic ray energy spectrum measured with 26 icetop stations
work_keys_str_mv AT collaborationi allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT abbasir allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT abdouy allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT abuzayyadt allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT ackermannm allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT adamsj allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT aguilarj allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT ahlersm allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT altmannd allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
AT andeenk allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
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AT bakerm allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
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AT beattiek allparticlecosmicrayenergyspectrummeasuredwith26icetopstations
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