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Fig. 15
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Transmission spectra of the Fe II lines at λ4522 Å, λ4583 Å, λ5018 Å, and λ5169 Å for KELT-9b (left column) and KELT-20b (right column) in comparison to the LTE (blue) and NLTE (green) synthetic profiles computed for the best fitting νmic and νmac values. The red line is the best Gaussian fit of the planetary signal.
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