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Fig. 4

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Comparison between the JWST/MIRI spectrum of B1-c (gray) and the lab spectra (colors) in the COM fingerprint range of 6.8–8.8 μm. Each panel focuses on one species and shows the comparison between the observed B1-c spectrum and the lab spectra with different mixing constituents, except for panel c, which shows the lab spectra of HCOO under different temperatures. The observed spectrum along with the 3σ level is shown in light gray, except for panel a, which blows up the CH4 band at ~7.7 μm, and the observed spectrum is plotted in black for clarity. In each panel, the spectrum in blue corresponds to the pure ice, and the best-fit spectrum to the observations is highlighted with a thicker red line. A similar comparison but for lab spectra under different temperatures is shown in Figs. 5 and C.1.

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