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Table 2
Summary of input and best-fit values for the ZDIPY and PIMMS codes, when applied to 100 simulated observations of a β Cep star with a dipolar magnetic field and uniform surface brightness, as described in Sect. 3.1.
| Parameter | Input | ZDIPY | PIMMS |
|---|---|---|---|
| vp,1 | 20.0000 | 20.0217 | |
| φ1 | 0.0000 | 0.0005 | |
| K1 | 0.0000 | 0.0000 | |
| vp,2 | 0.5000 | 0.4958 | |
| φ2 | 0.3000 | 0.3001 | |
| K2 | 0.0100 | 0.0109 | |
| vp,3 | 0.5000 | 0.5088 | |
| φ3 | 0.7000 | 0.7093 | |
| K3 | 0.1000 | 0.0754 | |
| Bd | 583 | 523 | 581 |
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