Table C.1.
Planet radius, in stellar radius units, obtained by our analysis as a function of wavelength (λc and bin width Δλ) for HD 189733b. The uncertainties in the radius correspond to a 68% confidence interval. For the analysis of the transmission spectrum, we subtracted 0.0277 Rp/R⋆ to match the average radius ratio of Pont et al. (2013).
| λc | Δλ | Rp/R⋆ | Uncertainty |
|---|---|---|---|
| 399.71 | 21.75 | 0.1871 | +0.0015/−0.0016 |
| 444.68 | 25.03 | 0.1850 | ±0.0011 |
| 494.75 | 26.69 | 0.1840 | ±0.0009 |
| 544.88 | 24.83 | 0.18178 | +0.0010/−0.0009 |
| 598.23 | 29.60 | 0.1832 | ±0.0011 |
| 658.695 | 24.925 | 0.1845 | ±0.0018 |
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