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Learning Path
Exoplanet Detection Methods → Case Study: Occurrence Rates from Kepler
This learning path guides graduate students through the essential statistical and domain knowledge needed to model exoplanet populations. It covers occurrence rate inference, detection bias correction, forward modeling, and Bayesian hierarchical models, culminating in the application of these methods to real exoplanet surveys.
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10 learning steps · 3 phases. Click any step to inspect it and see it on the Path Map.