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Perturbative analysis in planetary gravitational lensing
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The traditional perturbative method is applied to the case of gravitational lensing of planetary systems. A complete and detailed description of the structure of caustics for a system with an arbitrary number of planets can be obtained. I have also found precise analytical expressions for microlensing light curves perturbed by the presence of planets.
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Rate of caustic crossing microlensing events in stellar binary lenses with significant orbital motion
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