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. 2014 May 29;111(25):9042–9047. doi: 10.1073/pnas.1403473111

Fig. 5.

Fig. 5.

Characteristic transit spectrum for Titan showing both the signal for Titan transiting the Sun (left y axis) and the effective transit height (right y axis), assembled as a weighted mean of the four spectra in Fig. 4. The shaded region indicates uncertainty in our averaging, and is due to deviations from the mean in the four individual transit spectra. A best-fit haze model is shown (dashed).