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Table 4
Subjective (“eye”) and quantitative (“fit”) optimal solutions of our precession model using all the eclipses.
| Parameter | Eye | Fit | ± | Unit |
|
|
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| R d0 | 75.0 | 73.8 | 2.7 | R ⊙ |
| H | 1.0 | 0.6 | ... | R ⊙ |
| D | 4.0 | 4.0 | ... | R ⊙ |
| T 0 | 40493.92 | 40493.92 | ... | day |
| V t | 2.0 | 2.0 | ... | R⊙/day |
| θ d | 12.5 | 12.1 | 0.7 | degree |
| φ d * | 175.0 | 173.7 | 1.9 | degree |
| θ prec | 18.0 | 19.5 | 1.0 | degree |
| φ prec | 79.0 | 80.0 | 2.0 | degree |
| P prec | 11.8 | 10.8 | 0.4 | P orb |
| κ s | 0.328 | 0.328 | ... | 1 |
| ρ c | 1.18 | 1.13 | 1.21 | 1  |
| n ** | 0.3 | 0.27 | 0.09 | 1 |
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