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  • 13. Atmospheric neutrinos and discovery of neutrino oscillations.
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  • 14. Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory.
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  • 15. Observation of ultrahigh-energy cosmic rays with the ANITA balloon-borne radio interferometer.
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  • 16. Measurement of the depth of maximum of extensive air showers above 10{18} eV.
    Abraham J; Abreu P; Aglietta M; Ahn EJ; Allard D; Allekotte I; Allen J; Alvarez-Muñiz J; Ambrosio M; Anchordoqui L; Andringa S; Anticić T; Anzalone A; Aramo C; Arganda E; Arisaka K; Arqueros F; Asorey H; Assis P; Aublin J; Ave M; Avila G; Bäcker T; Badagnani D; Balzer M; Barber KB; Barbosa AF; Barroso SL; Baughman B; Bauleo P; Beatty JJ; Becker BR; Becker KH; Bellétoile A; Bellido JA; Benzvi S; Berat C; Bergmann T; Bertou X; Biermann PL; Billoir P; Blanch-Bigas O; Blanco F; Blanco M; Bleve C; Blümer H; Bohácová M; Boncioli D; Bonifazi C; Bonino R; Borodai N; Brack J; Brogueira P; Brown WC; Bruijn R; Buchholz P; Bueno A; Burton RE; Busca NG; Caballero-Mora KS; Caramete L; Caruso R; Castellina A; Catalano O; Cataldi G; Cazon L; Cester R; Chauvin J; Chiavassa A; Chinellato JA; Chou A; Chudoba J; Clay RW; Colombo E; Coluccia MR; Conceição R; Contreras F; Cook H; Cooper MJ; Coppens J; Cordier A; Cotti U; Coutu S; Covault CE; Creusot A; Criss A; Cronin J; Curutiu A; Dagoret-Campagne S; Dallier R; 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Tueros M; Ulrich R; Unger M; Urban M; Valdés Galicia JF; Valiño I; Valore L; van den Berg AM; Vázquez JR; Vázquez RA; Veberic D; Venters T; Verzi V; Videla M; Villaseñor L; Vorobiov S; Voyvodic L; Wahlberg H; Wahrlich P; Wainberg O; Warner D; Watson AA; Westerhoff S; Whelan BJ; Wieczorek G; Wiencke L; Wilczyńska B; Wilczyński H; Williams C; Winchen T; Winnick MG; Wundheiler B; Yamamoto T; Younk P; Yuan G; Yushkov A; Zas E; Zavrtanik D; Zavrtanik M; Zaw I; Zepeda A; Ziolkowski M;
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  • 17. Investigation of cosmic-ray induced background of Germanium gamma spectrometer using GEANT4 simulation.
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  • 18. Radio-frequency measurements of coherent transition and cherenkov radiation: implications for high-energy neutrino detection.
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