Skip to main content
. Author manuscript; available in PMC: 2020 May 5.
Published in final edited form as: Astrophys J Lett. 2018 Feb 20;854(2):L30. doi: 10.3847/2041-8213/aaadbd

Figure 3:

Figure 3:

(top) : Same as figure 2, but for a sample of fits in the 600–900 cm−1 part of the FP3 Titan spectrum : (top) December 2013 near 70°S; (middle) December 2013 near 70°N; (bottom) the same spectral region in August 2016 near 70°N. The feature close to 795 cm−1 not reproduced in the simulation corresponds to an interference pixel in the data that was not completely suppressed in some cases.