Fig. 2
Transit photometry of NGTS-14A from several instruments, offset vertically for clarity. From top to bottom: NGTS survey photometry (binned to two minutes in grey, binned to two minute equivalent in phase in blue); TESS (unbinned); Euler (binned to two minutes); SAAO (binned to two minutes); CHAT (unbinned); and single night NGTS multi-telescope observations(binned to two minutes). Our best fitting model is shown as a solid black line.
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