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Fig. B.4.

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Pre-explosion forced photometry at the location of SN 2022lxg from ZTF, ATLAS and ASAS-SN. Individual epochs have been binned per season. Non-detections are shown as downward-facing triangles. The peak time is shown as a dashed vertical line. No significant pre-explosion emission is detected for SN 2022lxg. The forced photometry rules out long-lasting precursors with absolute magnitude M ≲ −11 mag that might have happened within four years prior to explosion, but before that, they are not deep enough to rule out outbursts similar to those of other SNe.

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