Report of the Working Group on the Composition of Ultra-High Energy Cosmic RaysUnger, Michael (Avtor)
Filipčič, Andrej (Avtor)
Kukec Mezek, Gašper (Avtor)
Saleh, Ahmed (Avtor)
Stanič, Samo (Avtor)
Trini, Marta (Avtor)
Veberič, Darko (Avtor)
Vorobiov, Serguei (Avtor)
Yang, Lili (Avtor)
Zavrtanik, Danilo (Avtor)
Zavrtanik, Marko (Avtor)
Pierre Auger ObservatoryTelescope ArrayUltra-High Energy Cosmic Rayselemental compositionextensive air showersthe atmospheric depth of the air shower maximumThe atmospheric depth, Xmax, at which the particle number of
an air shower reaches its maximum is a good indicator for the
mass of the primary particle. We present a comparison of the
energy evolution of the mean of Xmax as measured by the
Telescope Array and c Collaborations. After
accounting for the different resolutions, acceptances and
analysis strategies of the two experiments, the two results are
found to be in good agreement within systematic uncertainties.20152016-03-08 14:40:16Delo ni kategorizirano2159COBISS_ID: 4158459NUK URN: URN:SI:UNG:REP:CV0X6NRCsl