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NGTS and WASP photometric recovery of a single transit candidate from TESS

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Figure

Figure 1. Difference imaging TESS light curve for TIC-238855958 (black)with best-fitting global model (red) and box used to detect the single-transitevent (blue dashed).
Figure 2. Results of template matching in archival WASP data for TIC-238855958. �χ2 is plotted as a function of time with peaks labelled with red circleswhen they meet the threshold level (red dashed)
Table 1. Stellar atmospheric parameters, orbital solution, and physicalproperties of the TIC-238855958 system
Figure 5. Mass–radius diagram for late M-dwarfs in eclipsing systems. Weplot the M-dwarf companion of TIC-238855958 in red, M-dwarfs measuredwithin the EBLM project in blue, and M-dwarfs with masses and radiiknown to better than 10 per cent (from table 4 o

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