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Fig. 11


Correlation between LIR and rest-frame luminosities at observed 10, 18, 21-, and 25.5 μm. The choice of the rest-frame luminosity wavelengths corresponds to the central wavelengths of the JWST-MIRI filters. Each IRS spectrum was shifted to the rest-frame and convolved with MIRI filters. The best-fit regression line and the associated plot are shown in each panel and are summarised in Table 3.

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