Explanations of four representative anomalies detected with different MSE-based scores, each showing the median normalized flux (top. with an SDSS imaging thumbnail) and corresponding maximum normalized LIME explanation weights (bottom). The panels show: (a) an extreme emission-line object driven by [OIII] and Hα peaks (MSE), (b) the red-end weighting from likely instrumental noise (MSE), (c) a broad emitter with high weights on Hα and [OII] (filtered MSE), and (d) continuum deviations near Hα and the 400 nm break (filtered + trimmed MSE). The explanations consistently highlight features driving the anomaly. This agrees with astronomers’ interpretations.