Biases in Orbital Fitting of Directly Imaged Exoplanets with Small Orbital Coverage
The eccentricity of a planet’s orbit and the inclination of its orbital plane encode important information about its formation and history. However, exoplanets detected via direct imaging are often only observed over a very small fraction of their period, making it challenging to perform reliable ph...
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Veröffentlicht in: | The Astronomical journal 2021-05, Vol.161 (5), p.241 |
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