Example of a simulated SPB star. The lower/left axes belong to the amplitude spectrum (blue line), where we have highlighted the mode frequencies (dotted lines), the first mode period (P₀), and the first period spacing (ΔP₀). The upper/right axes belong to the corresponding light curve (shown for the first 15 days) in its noise-less form (orange line) and simulated form (black points, representing a 𝓟 ≈ 10.3 star observed with n_CAM = 6).