Properties of Microlensing Light Curve Anomalies Induced by Multiple Planets

Cheongho Han; Heon-Young Chang; Jin H. An; Kyongae Chang

doi:10.1046/j.1365-8711.2001.04973.x

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arXiv · astro-ph/0107517

Properties of Microlensing Light Curve Anomalies Induced by Multiple Planets

Cheongho Han·Heon-Young Chang·Jin H. An·Kyongae Chang

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Abstract

In this paper, we show that the pattern of microlensing light curve anomalies induced by multiple planets are well described by the superposition of those of the single-planet systems where the individual planet-primary binary pairs act as independent lens systems. Since the outer deviation regions around the planetary caustics of the individual planets occur in general at different locations, we find that the pattern of anomalies in these regions are hardly affected by the existence of other planet(s). This implies that even if an event is caused by a multiple planetary system, a simple single-planet lensing model is good enough for the description of most anomalies caused by the source passage of the outer deviation regions. Detection of the anomalies resulting from the source trajectory passing both the outer deviation regions caused by more than two planets will provide a new channel of detecting multiple planets.

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Cheongho Han, Heon-Young Chang, Jin H. An, Kyongae Chang. 2001-07-27. Properties of Microlensing Light Curve Anomalies Induced by Multiple Planets. https://doi.org/10.1046/j.1365-8711.2001.04973.x

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