Closed hrwakeford closed 1 year ago
Be able to return uncertainty values for each of the limb-darkening coefficients computed from the stellar models, such that these can be used as prior ranges when fitting for LDCs in time series data.
Be able to return uncertainty values for each of the limb-darkening coefficients computed from the stellar models, such that these can be used as prior ranges when fitting for LDCs in time series data.