A new treatment of telluric and stellar features for medium-resolution spectroscopy and molecular mapping - Application to the abundance determination on β Pic b

Open Access

Fig. 7

Star flux fraction, $K_{i_{p}, ⋆}$ ${K_{{i_p}, \star }}$ at λ=2.165 µm (top panel). The corresponding planet flux fraction, $1 - K_{i_{p}, ⋆}$ $1 - {K_{{i_p}, \star }}$ , at the same wavelength (bottom panel). It can be seen that some background components contribute to the residuals.

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