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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 5.

Schematics of the used geometry. The impact point ρ (solid blue line) gets transferred to the camera plane along the green dashed line, if the muon is inclined (see the definition of ψ in Figure 1). The resulting impact distance with respect to the camera (dashed purple line) is denoted as ρ′. A possible hole in the center of the mirror support structure is drawn as a circle of radius r. The half-side length of the camera is denoted by A.

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