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The energy spectrum and mass composition of Ultra-High Energy Cosmic Rays (UHECRs) above 1018.2 eV from the Telescope Array (TA) utilizing 6 years of hybrid data are presented. TA is a hybrid experiment consisting of fluorescence detectors (FDs) and surface detectors (SDs). We have measured the energy spectrum and mass composition using a hybrid analysis technique which uses information from both FDs and SDs. The obtained energy spectrum with a 21% energy scale uncertainty is in agreement with the results of the HiRes experiment. The mass composition measurement performed by observing the depth of shower maximum (Xmax) is consistent with a light primary model.

Energy Spectrum and Mass Composition of Ultra-High Energy Cosmic Rays Measured by the hybrid technique in Telescope Array