AI 中文总结
本研究通过对比历史实验数据与奥格天文台光谱，发现历史数据支持奥格结果，而望远镜阵列与奥格之间的光谱差异依然未解。
AI 中文摘要
皮埃尔·奥格天文台和望远镜阵列合作组报告的能量谱之间的差异是众所周知的。为了理解这些差异，我们参照奥格合作组报告的光谱，研究了AGASA、Volcano Ranch和Haverah Park早期工作中测量的通量残差。在对踝区之前的能量进行经验性调整后（在该区域，两个半球的通量预计是相同的），发现历史数据与皮埃尔·奥格天文台在30 EeV以上的测量结果高度一致。因此，望远镜阵列与奥格天文台测量的光谱之间的张力仍然存在。
英文摘要
The differences between the energy spectra reported by the Pierre Auger Observatory and the Telescope Array Collaboration are well-known. In an effort to understand these differences, we have studied the residuals of the fluxes measured in early work at AGASA, Volcano Ranch and Haverah Park with reference to the spectrum reported by the Auger Collaboration. After an empirical adjustment to the energies in the region before the ankle, where fluxes from the two hemispheres are expected to be the same, it is found that historic data are in good agreement with measurements made at the Pierre Auger Observatory above 30 EeV. Thus, the tensions between the spectra measured by the Telescope Array and the Auger Observatory remain.
Comments8 pages, 8 figures, proceedings for ECRS2026
