Fig. 2
Photometry observations of NGTS-13. Top: NGTS observations (in 30-min bins for visual purposes), with the EXOFASTv2 model (see Sect. 3.2) in red. Middle: TESS FFI observations after the de-trending described in Sect. 2.2 was applied, with the EXOFASTv2 model in red. Bottom: NGTS in 30-min bins and TESS FFI photometry phased to the 4.12 day period of NGTS-13b. The NGTS data are in 30-min bins and then phased to the period. The red lines show the EXOFASTv2 model.
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