Fig. 6.
UV, optical and near-IR light curves of SN 2018bsz. All photometry is corrected for both Milky Way and host galaxy line of sight extinction. Epochs of optical spectroscopy are shown as blue lines on the x-axis, while epochs of near-IR spectroscopy are indicated by red lines. The upper limit of the most recent non-detection prior to discovery is shown as a maroon upside-down triangle.
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