Image Details

Choose export citation format:

A Heavy-metal Scenario of Ultra-high-energy Cosmic Rays

  • Authors: Jakub Vícha, Alena Bakalová, Ana L. Müller, Olena Tkachenko, Maximilian K. Stadelmaier

Jakub Vícha et al 2025 The Astrophysical Journal Letters 986 .

  • Provider: AAS Journals

Caption: Figure 2.

The relation between the interpreted moments of ﹩\mathrm{ln}A﹩ with (filled markers) and without (open markers) the application of ΔXmax to the model predictions using Auger DNN data (A. Abdul Halim et al. 2025a). The dashed and solid lines correspond to the systematic uncertainties. The range of possible combinations for p, He, N, and Fe nuclei is limited by the black lines forming the umbrella. The resulting value of ﹩{\sigma }^{2}(\mathrm{ln}A)﹩ inferred from the correlation coefficient rG between the ground signal and Xmax (A. Aab et al. 2016b) for 3–10 EeV is shown by the gray band, with the darker and narrower band indicating the respective energy range of the points for ΔXmax.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse