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MOPSS. II. Extreme Optical Scattering Slope for the Inflated Super-Neptune HATS-8b

  • Authors: E. M. May, T. Gardner, E. Rauscher, and J. D. Monnier

2020 The Astronomical Journal 159 7.

  • Provider: AAS Journals

Caption: Figure 3.

For our check star’s white light binning, here we show the following: (A) pixel shift in the spatial direction as a function of time, (B) pixel shift in the spectral direction as a function of time, (C) background counts as a function of time, (D) seeing as a function of time, and (E) airmass extinction corrected data with our red-noise model (see Equation (3)) over plotted. The red box represents the in-transit times and are not used in the fit but are predicted on.

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