Fig. B.2.
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Decomposition of the optical spectra of AT 2021hdr taken with the SPM in 2022 (top) and 2023 (bottom). The black corresponds to the original spectrum, the blue to the best-fitted model, the orange to the host galaxy contribution, the purple the continuum from the AGN emission, the green to the narrow emission lines (NELs), and the red to the broad emission lines (BELs).
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