Fig. 1
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Photometric light curves for NGTS-26. (a) Phase-folded light curve of NGTS-26 discovered with NGTS. The different colours correspond to individual transits. Dark points correspond to a binning of 22.3 min. (b) Phase-folded light curve of TESS, Sector 38 data, without dilution correction. The binning and colours are the same as for a. (c) EulerCam NGTS band, (d) SAAO I band, and (e) SAAO V band. The UT night of each observation is indicated on the plots c–e.
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