Figure 7 from Using Muon Rings for the Calibration of the Cherenkov Telescope Array: A Systematic Review of the Method and Its Potential Accuracy

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Using Muon Rings for the Calibration of the Cherenkov Telescope Array: A Systematic Review of the Method and Its Potential Accuracy

Authors: M. Gaug, S. Fegan, A.M.W. Mitchell, M.C. Maccarone, T. Mineo, and A. Okumura

2019 The Astrophysical Journal Supplement Series 243 11.

Provider: AAS Journals

Caption: Figure 7.

Left: line integration along the mirror surface as a function of azimuth angle for a given impact position, shown for the LST with the (still simplified, but more realistic) mirror profile (solid line) and under a circular approximation (dashed line). Right: modulation of the intensity profile along the ring for the given impact distance.

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