Fig. 3.
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Spectral series of SN 2022lxg (scaled with the photometry and corrected for MW extinction). Emission lines are marked with vertical dashed lines; throughout the evolution of SN 2022lxg, we detect Balmer lines, He Iλ5876, a broad blend of Fe II (∼5300 Å), and the Ca II NIR triplet. Other marked species are to guide the eye. Telluric features are indicated with grey shaded vertical lines.
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