Fig. C.2.
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Histograms of the line ratios obtained for each cluster per galaxy using the ch3-all cubes. Instead of regular histograms, we use KDEs for visualisation purposes, that compute continuous probability density curves. The red, dashed line marks the median values of the line ratios measured in Sy galaxies with MIRI/MRS by Zhang et al. (2024b) as a reference.
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