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A Gaussian process framework for modelling stellar activity signals in radial velocity data
Monthly Notices of the Royal Astronomical Society, no. 3 (2015): 2269-2291
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To date, the radial velocity (RV) method has been one of the most productive techniques for detecting and confirming extrasolar planetary candidates. Unfortunately, stellar activity can induce RV variations which can drown out or even mimic planetary signals – and it is notoriously difficult to model and thus mitigate the effects of these...更多
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