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Fig. 9

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Iron atmospheric model spectrum as a function of wavelength including contributions given by the hydride as a source of continuum absorption. In blue the atmospheric model for Fe, with no absorber added. In orange, the template spectrum including H free-free as source of continuum opacity, boosted by a factor of 10. In red, the spectrum including a solar amount of H bound-free. In the green and purple spectra, the bound-free contribution is boosted by a factor of 10 and 1000, respectively. The purple spectrum includes contributions by H2O beyond 1.6 μm. The grey and cyan coloured regions indicate HARPS and NIRPS coverage, respectively. It is worth mentioning that HARPS and NIRPS cover a similar fractional bandpass. We intentionally boost the continuum level differentiating the two main contributions to illustrate how the Fe spectrum changes accordingly.

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