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Table 3
Limb-darkening coefficients with the law 
(Claret 2000) and a star with solar parameters or for the ⟨3D⟩ profile of the RHD simulation (Fig. 2, green line) or the intensity profile of Hinode data (Fig. 7, green line).
| Reference | a1 | a2 | a3 | a4 | |||
|
|
|||||||
| Claret et al. (2000) | 0.5169 | –0.0211 | 0.6944 | –0.3892 | |||
| Magic et al. (2014) | 0.5850 | –0.1023 | 0.5371 | –0.2580 | |||
| Fit RHD ⟨3D⟩ | –3.8699 | 13.3547 | –15.4237 | 6.1910 | |||
| Fit Hinode data | 18.32 | –38.49 | 36.05 | –12.20 | |||
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