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Fig. 18

image

Modeling of TLC variability for an analogue of Kepler-15b with a prescribed precessing ring: panel a: model image of the transiting exoplanet with a precessing ring (solid line shows the trajectory of planet). Panel b: variations of the shape parameter As of the simulated synthetic TLC. Panel c: variations of the simulated transit duration Δte − Δts. Panel d: variations of the simulated transit depth ΔFtr. Panel e: variations of the simulated TLC minimum time Δtm. Panel f: variations of the simulated transit start-time Δts. Panel g: variations of the simulated transit end-time Δte. The abscissascale ΔJD = JD − 2 454 833.0 is in Julian days (JD).

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