Extended Data Fig. 5: Penetration depth of the direct and scattered flux for NIRSpec as a function of wavelength.
From: The atmosphere of Titan in late northern summer from JWST and Keck observations
Calculations at three emission angles: θe = 0∘ (nadir viewing, green), θe = 44∘ (red) and θe = 90∘ (limb viewing, blue).
