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Using Muon Rings for the Calibration of the Cherenkov Telescope Array: An Analytical Solution for the Dual-mirror Telescope Using Vector Geometry

  • Authors: Markus Gaug, Víctor Giráldez-Segalàs, Fiona Redmen

Markus Gaug et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 7.

Muon baffle-crossing conditions (Equation (38) and (39)) shown for muons with different normalized impact distances ρR and impact angles ϕ0, for the parameters of an SCT. In the left panel, the muon is inclined toward the left (ψ = 0°) with varying inclination angles ν, in the central panel, it is inclined toward the right (ψ = 180°), and in the right panel the inclination angle is fixed at ν = 4°, while the azimuthal projection ψ varies. Note that the azimuthal axis represents here the muon angle ϕ0, whereas in the previous figures the photon emission angle ϕ − ϕ0 was used. The gray shaded region in the center indicates the central hole in the primary mirror.

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