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    Aguilar M; Aisa D; Alpat B; Alvino A; Ambrosi G; Andeen K; Arruda L; Attig N; Azzarello P; Bachlechner A; Barao F; Barrau A; Barrin L; Bartoloni A; Basara L; Battarbee M; Battiston R; Bazo J; Becker U; Behlmann M; Beischer B; Berdugo J; Bertucci B; Bigongiari G; Bindi V; Bizzaglia S; Bizzarri M; Boella G; de Boer W; Bollweg K; Bonnivard V; Borgia B; Borsini S; Boschini MJ; Bourquin M; Burger J; Cadoux F; Cai XD; Capell M; Caroff S; Casaus J; Cascioli V; Castellini G; Cernuda I; Cervelli F; Chae MJ; Chang YH; Chen AI; Chen H; Cheng GM; Chen HS; Cheng L; Chikanian A; Chou HY; Choumilov E; Choutko V; Chung CH; Clark C; Clavero R; Coignet G; Consolandi C; Contin A; Corti C; Coste B; Crispoltoni M; Cui Z; Dai M; Delgado C; Della Torre S; Demirköz MB; Derome L; Di Falco S; Di Masso L; Dimiccoli F; Díaz C; von Doetinchem P; Donnini F; Du WJ; Duranti M; D'Urso D; Eline A; Eppling FJ; Eronen T; Fan YY; Farnesini L; Feng J; Fiandrini E; Fiasson A; Finch E; Fisher P; Galaktionov Y; Gallucci G; García B; García-López R; Gargiulo C; Gast H; Gebauer I; Gervasi M; Ghelfi A; Gillard W; Giovacchini F; Goglov P; Gong J; Goy C; Grabski V; Grandi D; Graziani M; Guandalini C; Guerri I; Guo KH; Habiby M; Haino S; Han KC; He ZH; Heil M; Hoffman J; Hsieh TH; Huang ZC; Huh C; Incagli M; Ionica M; Jang WY; Jinchi H; Kanishev K; Kim GN; Kim KS; Kirn T; Kossakowski R; Kounina O; Kounine A; Koutsenko V; Krafczyk MS; Kunz S; La Vacca G; Laudi E; Laurenti G; Lazzizzera I; Lebedev A; Lee HT; Lee SC; Leluc C; Li HL; Li JQ; Li Q; Li Q; Li TX; Li W; Li Y; Li ZH; Li ZY; Lim S; Lin CH; Lipari P; Lippert T; Liu D; Liu H; Lomtadze T; Lu MJ; Lu YS; Luebelsmeyer K; Luo F; Luo JZ; Lv SS; Majka R; Malinin A; Mañá C; Marín J; Martin T; Martínez G; Masi N; Maurin D; Menchaca-Rocha A; Meng Q; Mo DC; Morescalchi L; Mott P; Müller M; Ni JQ; Nikonov N; Nozzoli F; Nunes P; Obermeier A; Oliva A; Orcinha M; Palmonari F; Palomares C; Paniccia M; Papi A; Pauluzzi M; Pedreschi E; Pensotti S; Pereira R; Pilo F; Piluso A; Pizzolotto C; Plyaskin V; Pohl M; Poireau V; Postaci E; Putze A; Quadrani L; Qi XM; Räihä T; Rancoita PG; Rapin D; Ricol JS; Rodríguez I; Rosier-Lees S; Rozhkov A; Rozza D; Sagdeev R; Sandweiss J; Saouter P; Sbarra C; Schael S; Schmidt SM; Schuckardt D; Schulz von Dratzig A; Schwering G; Scolieri G; Seo ES; Shan BS; Shan YH; Shi JY; Shi XY; Shi YM; Siedenburg T; Son D; Spada F; Spinella F; Sun W; Sun WH; Tacconi M; Tang CP; Tang XW; Tang ZC; Tao L; Tescaro D; Ting SC; Ting SM; Tomassetti N; Torsti J; Türkoğlu C; Urban T; Vagelli V; Valente E; Vannini C; Valtonen E; Vaurynovich S; Vecchi M; Velasco M; Vialle JP; Wang LQ; Wang QL; Wang RS; Wang X; Wang ZX; Weng ZL; Whitman K; Wienkenhöver J; Wu H; Xia X; Xie M; Xie S; Xiong RQ; Xin GM; Xu NS; Xu W; Yan Q; Yang J; Yang M; Ye QH; Yi H; Yu YJ; Yu ZQ; Zeissler S; Zhang JH; Zhang MT; Zhang XB; Zhang Z; Zheng ZM; Zhuang HL; Zhukov V; Zichichi A; Zimmermann N; Zuccon P; Zurbach C;
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  • 15. Detection of spectral hardenings in cosmic-ray boron-to-carbon and boron-to-oxygen flux ratios with DAMPE.
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  • 16. Electron and positron fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the international space station.
    Aguilar M; Aisa D; Alvino A; Ambrosi G; Andeen K; Arruda L; Attig N; Azzarello P; Bachlechner A; Barao F; Barrau A; Barrin L; Bartoloni A; Basara L; Battarbee M; Battiston R; Bazo J; Becker U; Behlmann M; Beischer B; Berdugo J; Bertucci B; Bigongiari G; Bindi V; Bizzaglia S; Bizzarri M; Boella G; de Boer W; Bollweg K; Bonnivard V; Borgia B; Borsini S; Boschini MJ; Bourquin M; Burger J; Cadoux F; Cai XD; Capell M; Caroff S; Casaus J; Cascioli V; Castellini G; Cernuda I; Cervelli F; Chae MJ; Chang YH; Chen AI; Chen H; Cheng GM; Chen HS; Cheng L; Chikanian A; Chou HY; Choumilov E; Choutko V; Chung CH; Clark C; Clavero R; Coignet G; Consolandi C; Contin A; Corti C; Coste B; Cui Z; Dai M; Delgado C; Della Torre S; Demirköz MB; Derome L; Di Falco S; Di Masso L; Dimiccoli F; Díaz C; von Doetinchem P; Du WJ; Duranti M; D'Urso D; Eline A; Eppling FJ; Eronen T; Fan YY; Farnesini L; Feng J; Fiandrini E; Fiasson A; Finch E; Fisher P; Galaktionov Y; Gallucci G; García B; García-López R; Gast H; Gebauer I; Gervasi M; Ghelfi A; Gillard W; Giovacchini F; Goglov P; Gong J; Goy C; Grabski V; Grandi D; Graziani M; Guandalini C; Guerri I; Guo KH; Habiby M; Haino S; Han KC; He ZH; Heil M; Hoffman J; Hsieh TH; Huang ZC; Huh C; Incagli M; Ionica M; Jang WY; Jinchi H; Kanishev K; Kim GN; Kim KS; Kirn T; Kossakowski R; Kounina O; Kounine A; Koutsenko V; Krafczyk MS; Kunz S; La Vacca G; Laudi E; Laurenti G; Lazzizzera I; Lebedev A; Lee HT; Lee SC; Leluc C; Li HL; Li JQ; Li Q; Li Q; Li TX; Li W; Li Y; Li ZH; Li ZY; Lim S; Lin CH; Lipari P; Lippert T; Liu D; Liu H; Lomtadze T; Lu MJ; Lu YS; Luebelsmeyer K; Luo F; Luo JZ; Lv SS; Majka R; Malinin A; Mañá C; Marín J; Martin T; Martínez G; Masi N; Maurin D; Menchaca-Rocha A; Meng Q; Mo DC; Morescalchi L; Mott P; Müller M; Ni JQ; Nikonov N; Nozzoli F; Nunes P; Obermeier A; Oliva A; Orcinha M; Palmonari F; Palomares C; Paniccia M; Papi A; Pedreschi E; Pensotti S; Pereira R; Pilo F; Piluso A; Pizzolotto C; Plyaskin V; Pohl M; Poireau V; Postaci E; Putze A; Quadrani L; Qi XM; Rancoita PG; Rapin D; Ricol JS; Rodríguez I; Rosier-Lees S; Rozhkov A; Rozza D; Sagdeev R; Sandweiss J; Saouter P; Sbarra C; Schael S; Schmidt SM; Schuckardt D; Schulz von Dratzig A; Schwering G; Scolieri G; Seo ES; Shan BS; Shan YH; Shi JY; Shi XY; Shi YM; Siedenburg T; Son D; Spada F; Spinella F; Sun W; Sun WH; Tacconi M; Tang CP; Tang XW; Tang ZC; Tao L; Tescaro D; Ting SC; Ting SM; Tomassetti N; Torsti J; Türkoğlu C; Urban T; Vagelli V; Valente E; Vannini C; Valtonen E; Vaurynovich S; Vecchi M; Velasco M; Vialle JP; Wang LQ; Wang QL; Wang RS; Wang X; Wang ZX; Weng ZL; Whitman K; Wienkenhöver J; Wu H; Xia X; Xie M; Xie S; Xiong RQ; Xin GM; Xu NS; Xu W; Yan Q; Yang J; Yang M; Ye QH; Yi H; Yu YJ; Yu ZQ; Zeissler S; Zhang JH; Zhang MT; Zhang XB; Zhang Z; Zheng ZM; Zhuang HL; Zhukov V; Zichichi A; Zimmermann N; Zuccon P; Zurbach C;
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  • 17. Evidence of a Hardening in the Cosmic Ray Proton Spectrum at around 166 TeV Observed by the GRAPES-3 Experiment.
    Varsi F; Ahmad S; Chakraborty M; Chandra A; Dugad SR; Goswami UD; Gupta SK; Hariharan B; Hayashi Y; Jagadeesan P; Jain A; Jain P; Kawakami S; Kojima H; Lipari P; Mahapatra S; Mohanty PK; Moharana R; Muraki Y; Nayak PK; Nonaka T; Oshima A; Pant BP; Pattanaik D; Paul S; Pradhan GS; Rameez M; Ramesh K; Reddy LV; Saha S; Sahoo R; Scaria R; Shibata S; Zuberi M;
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  • 18. Towards Understanding the Origin of Cosmic-Ray Electrons.
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  • 19. Measurements of cosmic-ray proton and helium spectra from the BESS-Polar long-duration balloon flights over Antarctica.
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  • 20. Cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV.
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