Characterisation of TOI-406 as a showcase of the THIRSTEE program - A two-planet system straddling the M-dwarf density gap

Open Access

Fig. 3

ASAS-SN photometry of TOI-406 in V and g filters. Right panel: GLS periodogram of ASAS-SN photometry. The horizontal dashed and dotted lines represent the FAP level of 1% and 10%, respectively. The vertical red line shows the most significant peak.

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