Roadmap

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João Faria edited this page Jan 21, 2019 · 4 revisions

What kima will do in the future

Analyse RV observations from multiple spectrographs
- fit their respective systemic velocities
- fit individual white noise terms
Use more GP kernels, other than the quasi-periodic
- to model long-term magnetic activity cycles
- to model instrument systematics?
Any other ideas? You can help!

This documentation was created with ❤️ by @j-faria and @jdavidrcamacho, at IA.