Fig. 4.
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Mock ELT/HARMONI spectra focusing on the strongest lines detectable in the mock JWST/NIRSpec spectra. Both figures illustrate that features will be distinguishable in ELT/HARMONI spectra for fainter stars, and with shorter exposure times (5 hours for the left figure and 10 hours for the right one) than for JWST/NIRSpec. To clarify which lines are marked in the right figure, the areas encompassing the P Cygni profiles are filled.
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