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Fig. 7

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Element abundance determination of Gl 486 b. Top panel: coadded, order-merged, channel-merged CARMENES VIS (blue) and NIR (red) template spectrum. Interruptions (grey areas) are due to strong telluric contamination and inter-order and NIR detector array gaps. Bottom panels: zoomed-in view of six representative, weakly magnetic-sensitive atomic lines from Abia et al. (2020, Rb i, Sr ii), Shan et al. (2021, V i), Passegger et al. (2019, Mg i), and Marfil et al. (2021, Fe i, Ti i). Black dashed lines are the synthetic fits.

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