MINDS. Hydrocarbons detected by JWST/MIRI in the inner disk of Sz28 consistent with a high C/O gas-phase chemistry

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Fig. A.1

Stellar contribution to the JWST-MIRI/MRS spectrum. Top panel: JWST-MIRI/MRS spectrum of Sz28 and the modelled stellar spectrum, which has an offset of 0.009 Jy. Bottom panel: CO and H₂O absorption slabs and the continuum-subtracted JWST-MIRI/MRS spectrum, highlighting their respective presence.

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