Simulated performance of the molecular mapping for young giant exoplanets with the Medium-Resolution Spectrometer of JWST/MIRI

Open Access

Fig. 7

Signal-to-noise ratio obtained at each separation from the star for a range of planet’s temperature for the following molecules H₂O, CO. CH₄, HCN, NH₃, PH₃ (in the band or channel where the spectral features are the strongest), the cross represents simulation without any star.

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