Figure 11 from 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

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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 11.

Duration vs. phase for the Kepler-47b transits. The red curve represents a fit from Equation (4). The analytic expression recovers the parameters of the binary star very well— M _{bin, calc} = 1.35 M _☉ vs. 1.4 M _☉ and R _prim = 0.87 R _☉ vs. 0.96 R _☉ respectively, provided by Orosz et al. (2012a).

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