Image Details
Caption: Figure 5.
Spectral light-curve fits from Iraclis for the transmission spectra of LHS 1140b where, for clarity, an offset has been applied. In each plot, left panel: the detrended spectral light curves with best-fit model plotted; right panel: residuals from the fitting with values for the chi-squared (χ2), the standard deviation with respect to the photon noise (﹩\bar{\sigma }﹩), and the autocorrelation (AC).
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