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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 6.

Eclipse timing variations of the primary eclipses of KIC 4862625 (filled circles). The observed times of each primary eclipse minus the calculated times for a linear ephemeris are shown vs. time (an " O −  C" diagram). The nine planetary transit events are indicated by vertical dashed lines. A single primary eclipse is missing from the sequence at BJD = 2,455,567.8 and another, at BJD = 2,455,947.8, is incomplete. For comparison, two simulated " O −  C" variations are also shown, one for a 1  M J (squares) and the other for a 5  M J (diamonds) respectively, and shifted vertically for clarity. Evidently, the circumbinary body's mass is less than 5  M J.

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