Extended Data Fig. 1: G102 white-light curve and broadband spectroscopic light curves covering the wavelength range 0.88–1.14 μm for WASP-107b. | Nature

Extended Data Fig. 1: G102 white-light curve and broadband spectroscopic light curves covering the wavelength range 0.88–1.14 μm for WASP-107b.

From: Helium in the eroding atmosphere of an exoplanet

Extended Data Fig. 1

a, Relative flux of the white-light curve with respect to systematics model results (blue points), with the best-fitting transit light curve plotted in black. b, White-light residuals and 1σ errors, after removing the combined transit and systematics components of the best-fitting model. c, Points are spectroscopic light curves divided by systematics model results, and black curves are best-fitting transit models, with vertical offsets applied for clarity. d, Best-fitting spectroscopic model residuals, with vertical offsets applied for clarity. Differently coloured points in c and d are used to highlight separate channels.

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