The Auger and TA experiments use different fluorescence yields for shower reconstruction. The corresponding effect on their relative energy scales is studied. Simple analytical calculations show that the energy reconstructed by the TA telescopes should be larger than that of Auger. A detailed simulation has provided a more realistic evaluation of this effect showing similar results. Our analysis indicates that, if we neglect other contributions, the discrepancy in the energy scales due to the fluorescence yield would be of about 17%
The absolute value of the air-fluorescence yield is a key parameter for the energy reconstruction of...
The performance of the Auger Fluorescence telescope is discussed on the basis of a mass production c...
Abstract: The optical calibration of the fluorescence telescopes is a significant contribution to th...
The fluorescence yield data used for shower reconstruction in the Auger, HiRes and TA experiments ar...
The fluorescence yield data used for shower reconstruction in the Auger, HiRes and TA experiments ar...
Abstract: The energy scale of the Pierre Auger Observatory is derived from fluorescence observations...
The fluorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indi...
An accurate knowledge of the fluorescence yield and its dependence on atmospheric properties such as...
Abstract: The fluorescence yield is the key parameter that allows fluorescence telescope experiments...
Abstract: In order to investigate the effects of the fluorescence energy error distributions on the ...
This work investigates the processes used to reconstruct extensive air showers induced in the atmosp...
The energy spectrum of ultra-high energy cosmic rays is the most emblematic observable for describin...
Abstract A method to determine the primary energy of very rare big extensive air showers is to measu...
Abstract: Fluorescence telescopes are used for the calorimetric measurement of the energy of air sho...
Abstract: The composition of cosmic rays at the highest energies is one of the most important proble...
The absolute value of the air-fluorescence yield is a key parameter for the energy reconstruction of...
The performance of the Auger Fluorescence telescope is discussed on the basis of a mass production c...
Abstract: The optical calibration of the fluorescence telescopes is a significant contribution to th...
The fluorescence yield data used for shower reconstruction in the Auger, HiRes and TA experiments ar...
The fluorescence yield data used for shower reconstruction in the Auger, HiRes and TA experiments ar...
Abstract: The energy scale of the Pierre Auger Observatory is derived from fluorescence observations...
The fluorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indi...
An accurate knowledge of the fluorescence yield and its dependence on atmospheric properties such as...
Abstract: The fluorescence yield is the key parameter that allows fluorescence telescope experiments...
Abstract: In order to investigate the effects of the fluorescence energy error distributions on the ...
This work investigates the processes used to reconstruct extensive air showers induced in the atmosp...
The energy spectrum of ultra-high energy cosmic rays is the most emblematic observable for describin...
Abstract A method to determine the primary energy of very rare big extensive air showers is to measu...
Abstract: Fluorescence telescopes are used for the calorimetric measurement of the energy of air sho...
Abstract: The composition of cosmic rays at the highest energies is one of the most important proble...
The absolute value of the air-fluorescence yield is a key parameter for the energy reconstruction of...
The performance of the Auger Fluorescence telescope is discussed on the basis of a mass production c...
Abstract: The optical calibration of the fluorescence telescopes is a significant contribution to th...