Fig. 4
Fluxes (left) and absolute errors in fluxes (right) for the night side P–T profile in Fig. 3. The line-by-line (LbL) calculation was run at a 0.001 cm-1 resolution corresponding to 5 × 107 monochromatic calculations, while we used 120 rebinned k-coefficients in each band corresponding to 3840 pseudo-monochromatic calculations. Both results were obtained using ATMO.
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