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In this paper, we report the evidence for a planetary mass body orbiting theclose binary star KIC 5095269. This detection arose from a search for eclipsetiming variations among the more than 2,000 eclipsing binaries observed byKepler. Light curve and periodic eclipse time variations have been analysedusing Systemic and a custom Binary Eclipse Timings code based on the TransitAnalysis Package which indicates a $7.70\pm0.08M_{Jup}$ object orbiting every$237.7\pm0.1d$ around a $1.2M_\odot$ primary and $0.51M_\odot$ secondary in an18.6d orbit. A dynamical integration over $10^7$ years suggests a stableorbital configuration. Radial velocity observations are recommended to confirmthe properties of the binary star components and the planetary mass of thecompanion.

Evidence for a planetary mass third body orbiting the binary star KIC 5095269