Figure 13 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 13.

Mass of the binary ( M _A + M _B ) derived using the results from the RV measurements and applying Equation (4) to 10,000 iterations of the nine planetary transit durations, scrambled and with added normalized noise with σ = 1 hr. We used this distribution to set the limits of our search space for the primary mass in our dynamical model of KIC 4862625.

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