Fig. 8
Eclipse depth, in ppm, as a function of wavelength. Literature values are taken from Croll et al. (2015); Beatty et al. (2014, 2017, 2019). Our new data point is plotted in red. The gray area shows a 1σ contour of the equilibrium temperature of KELT-1b, determined from all data. Transmission responses are plotted in black continuous lines, with the exception of TESS, highlighted in red.
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