Fig. 10
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Spectral comparison between Spitzer IRS observations (Suárez & Metchev 2022) and our JWST MIRI LRS observations for 2M0355+11 and 2M2244+20. The Spitzer spectra are shown in black and our spectra are coloured. Top two panels: Comparison for 2M0355+11. Bottom two panels: Comparison for 2M2244+20. The uncertainties are shown as the shaded envelope region. Below each spectral comparison is the relative flux difference (max/min − 1).
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