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Fig. 4.


Comparison of AT 2018hso with three ILRTs (dashed lines): SN 2008S, NGC300-2008OT1 (Humphreys et al. 2011), and AT 2017be, and two LRNe (solid lines): AT 2017jfs, NGC4490-2011OT1. Top: black-body temperature evolution. Middle: bolometric light curves. Bottom: evolution of the photospheric radii.

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