HOW LOW CAN YOU GO? THE PHOTOECCENTRIC EFFECT FOR PLANETS OF VARIOUS SIZES

@article{Price2014HOWLC,
  title={HOW LOW CAN YOU GO? THE PHOTOECCENTRIC EFFECT FOR PLANETS OF VARIOUS SIZES},
  author={Ellen M. Price and Leslie A. Rogers and John Asher Johnson and Rebekah I. Dawson},
  journal={The Astrophysical Journal},
  year={2014},
  volume={799}
}
It is well-known that the light curve of a transiting planet contains information about the planet's orbital period and size relative to the host star. More recently, it has been demonstrated that a tight constraint on an individual planet's eccentricity can sometimes be derived from the light curve via the “photoeccentric effect,” the effect of a planet's eccentricity on the shape and duration of its light curve. This has only been studied for large planets and high signal-to-noise scenarios… 

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