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A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the Two Transiting Planets in the Kepler-47 System

  • Authors: V. B. Kostov, P. R. McCullough, T. C. Hinse, Z. I. Tsvetanov, G. Hébrard, R. F. Díaz, M. Deleuil, and J. A. Valenti

Kostov et al. 2013 The Astrophysical Journal 770 52.

  • Provider: AAS Journals

Caption: Figure 5.

Kepler light curves of KIC 4862625. The normalized and detrended flux of the primary and secondary eclipses is shown with respect to the orbital phase of the EB, along with the binary star model. The secondary eclipse data have been centered at zero phase for comparison with the primary eclipse data. The secondary eclipse data and the residuals (above) have been offset vertically for clarity.

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