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Table 1

MOCKA’s arsenal of pressure (p) and gravity (𝑔) mode pulsators.

Variability Spectral Dominant Typical N 𝒫max δt
class type mode character periods [mag] [s]
Cepheid (Ceph) F6-K2 Low-order, radial p modes 1–300 day 2000 17 600
RR Lyrae (RR Lyr) F0-G9 Low-order, radial p modes 0.3–1.0 day 2000 17 600
Slowly pulsating B (SPB) B3-B9 High-order, non-radial 𝑔 modes 0.2–3.2 day 4000 16 600
γ Doradus (γ Dor) F4-F0 High-order, non-radial 𝑔 modes 0.2–3.0 day 4000 14 600
β Cephei (β Cep) O8-B6 Low-order, p- and 𝑔 modes 2.5–8.0 hour 2000 16 50
δ Scuti (δ Sct) A0-F5 Low-order, non-radial p modes 0.2–8.0 hour 4000 16 50
sdBV (V361 Hya, V1093 Her) B0-B9 Non-radial p- and 𝑔 modes 1–180 min 17 × 10 17 25
White dwarf (WD: DA, DB, DO) D(OBA) High-order, non-radial 𝑔 modes 0.5–25 min 30 × 10 17 25

Notes. First four columns display generic information about each pulsating class. Last three columns show the number of stars (N), the limiting magnitude (𝒫max), and the final cadence (δt) of each sample simulated.

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