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
Hauptverfasser: Ferrer-Chávez, Rodrigo, Wang, Jason J., Blunt, Sarah
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Sprache:eng
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