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Fig. 8

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Example of the reference optical depth and wavelength of the ODF points organised into bins for the F3V, G2V, K0V, and M2V stars. As explained in the text, the Rosseland optical depth shown in the vertical axis is used as the reference τref(zi,j), where zi,j is the geometrical height at which τi,j = 1 for each step and substep of the ODF. We show the same {τ, λ} binning configuration for all the stars. The colours indicate different bins. Each point corresponds to one ODF substep, all centred in the middle wavelength of their corresponding step. The last column of dots at the right of each panel corresponds to the ODF step with λ ∈ [9600, 9.5 × 104] nm, and thus, appears separated from the rest of the dots.

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