Figure 3 from A Population Study of Gaseous Exoplanets

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A Population Study of Gaseous Exoplanets

Authors: A. Tsiaras, I. P. Waldmann, T. Zingales, M. Rocchetto, G. Morello, M. Damiano, K. Karpouzas, G. Tinetti, L. K. McKemmish, J. Tennyson, and S. N. Yurchenko

2018 The Astronomical Journal 155 156.

Provider: AAS Journals

Caption: Figure 3.

Standard deviation (top) and autocorrelation (bottom) of the fitting. These metrics indicate that while the white light curves (blue) are subjected to remaining signals in their residuals, the divide-white method used here is efficient in removing those signals from the spectral light curves (red).

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