Table 8
Radius and uncertainty due to the granulation fluctuations for the different prototype planets of Table 3 and 3D RHD simulations of Table 1.
Planet | Star | Wavelength | Radius max/min | Radius 1σ |
[Å] | [%] | [%] | ||
|
||||
terrestrial | Sun | [7600–7700] | 0.90 | 0.40 |
Neptune | 0.43 | 0.29 | ||
hot Jupiter | 0.47 | 0.36 | ||
|
||||
terrestrial | [25 000–29 000] | 0.35 | 0.13 | |
Neptune | 0.22 | 0.11 | ||
hot Jupiter | 0.08 | 0.05 | ||
|
||||
terrestrial | [39 000–51 000] | 0.20 | 0.11 | |
Neptune | 0.15 | 0.07 | ||
hot Jupiter | 0.10 | 0.10 | ||
|
||||
terrestrial | K dwarf | [7600–7700] | 0.58 | 0.22 |
Neptune | 0.45 | 0.23 | ||
hot Jupiter | 0.45 | 0.21 | ||
|
||||
terrestrial | [25 000–29 000] | 0.27 | 0.18 | |
Neptune | 0.10 | 0.07 | ||
hot Jupiter | 0.07 | 0.04 | ||
|
||||
terrestrial | [39 000–51 000] | 0.16 | 0.09 | |
Neptune | 0.10 | 0.05 | ||
hot Jupiter | 0.07 | 0.04 |
Notes. The values reported have been computed for transit points covering the central part of the transit periods: [−1, +1] h for terrestrial planet, [−0.2, +0.2] h for the hot Neptune, and [−0.15, +0.15] h for the hot Jupiter. These values are representative for all the wavelength bands from Table 2. Column 4 shows the radius uncertainty computed for transit depth values between the maximum and minimum transit fluctuations, while Col. 5 lists this for transit depth values between 1σ uncertainty (see Fig. 13).
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