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A study of the systematic effects on the energy scale for the measurement of UHECR spectrum by the TA SD array
We evaluated the systematic deviation of energy scales for the energy spectrum of the highest energy cosmic rays observed by the Telescope Array Surface Detector array due to differences in atmospheric fluorescence yield and missing energy estimation. The energy dependence on the energy scales is also investigated and observationally confirmed by the constant intensity cut method analysis. The results of these studies will be presented.
- University of Tokyo Japan
- University of California, Santa Cruz United States
- University of Nova Gorica Slovenia
- Institute for Cosmic Ray Research Japan
- Institute for Cosmic Ray Research Japan
fluorescence yield, Telescope Array, ground array, cosmic rays, fluorescence detection, energy spectrum, ultra-high energy, indirect detection, info:eu-repo/classification/udc/52, systematics, surface detection, missing energy
fluorescence yield, Telescope Array, ground array, cosmic rays, fluorescence detection, energy spectrum, ultra-high energy, indirect detection, info:eu-repo/classification/udc/52, systematics, surface detection, missing energy
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).0 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Average influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Average impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Average
