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Table 2.
Summary of the seismic simulation.
| Steps | Input | Output | Equations | |
|---|---|---|---|---|
| [0] | νmax from stellar parameters | M, R, Teff, or log g | νmax | (1) |
| [1.1] | Oscillation signal and granulation background | νmax | Hmax, Bmax | (4), (5) |
| [1.2] | Instrumental noise | m, Bsys, Bpho, Badd | Bnoise | (6) + Table 1 |
| [1.3] | Height-to-background ratio | Hmax, Bmax, Bnoise | ℛ | (3) |
| [2.1H] | Raw performance index (≤RGB stage) | ℛ, νmax, 𝒟 | ℰ | (7) |
| [2.1He] | Raw performance index (≥RC stage) | ℛ, νmax, 𝒟 | ℰ | (8) |
| [2.2] | Damping close to the instability strip | M, Teff, νmax | κ | (9) |
| [2.3] | Seismic index | ℰ, κ | ℰκ = κ ℰ | |
| [3.1] | Detection threshold | νmax | ℰdet | (12) |
| [3.2] | Thresholds: evolutionary stage, rotation | νmax | ℰmix, ℰΔΠ, ℰrot | (13)–(15) |
| [3.3] | Thresholds: relative mass uncertainty | νmax, xM | ℰM | (21) |
| [4.1] | Positive seismic detection | ℰκ, ℰdet | ℰκ ≥ ℰdet | |
| [4.2] | Seismic performance | ℰκ, ℰmix, ℰΔΠ, ℰrot, ℰM | ℰκ ≥ ℰmix, or ℰκ ≥ … | |
Notes. The independent variables are the stellar parameters M, R, Teff, the stellar magnitude m, the instrumental noise contributions Bsys, Bpho and Badd, and the observation length 𝒟 (see Table 3).
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