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Fig. 9


Transit timing variatons caused by a hypothetical P2 = 10   000 day-period m3 = 0.005   M( ≈ 5   MJ) mass third companion for HD 80606b at the maximum eccentricity phase of the induced Kozai-cycles. Top: e2 = 0; middle: e2 = 0.3; bottom: e2 = 0.7 (g2 = 0° in all cases); left panels: primary transits; middle panels: secondary occultations; right panels: primary minus secondary difference. See text for further details. (For better comparison the curves are corrected for the different average transit periods, and zero point shifts.)

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