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Fig. 6

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Average spectra and LIME explanation weights for cluster 3 of the top 1% most anomalous spectra (MSE score). Cluster 3 is dominated by [O III]λ500.7, which is characteristic of extreme low-metallicity systems. As discussed for clusters 1 and 2, clustering by explanation profiles reveals distinct physical regimes within spectrally similar galaxies. The fluxes are median normalized.

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