Disentangling the dust and gas contributions of the JWST/MIRI spectrum of Sz 28

Open Access

Fig. 3

Zoom in on the isotopologue features comparing the version with all isotopologues (grey) with the ones excluding ¹³CH₄, ¹³CCH₆, ¹³CCH₂, and ¹³CO₂, respectively. While the JWST/MIRI spectrum is shown in 1σ, 2σ, and 3σ flux levels of the posteriors are displayed in lighter growing shades of their respective colours.

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