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={E. M. Price and L. Rogers and J. Johnson and R. Dawson},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2014}
}
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… Expand

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References

SHOWING 1-10 OF 40 REFERENCES
A Unique Solution of Planet and Star Parameters from an Extrasolar Planet Transit Light Curve
Transit Light Curves with Finite Integration Time: Fisher Information Analysis
A rocky composition for an Earth-sized exoplanet
An Earth-sized planet with an Earth-like density
A map of the day–night contrast of the extrasolar planet HD 189733b
Impact of Orbital Eccentricity on the Detection of Transiting Extrasolar Planets
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