A non-parametric Gaia DR3 membership method finds more member stars in 21 rich open clusters than previous catalogs, and Bayesian isochrone fits yield age, metallicity, distance, and reddening posteriors.
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Open Cluster Study Using $Gaia$ I:Membership and Cluster Properties
A non-parametric Gaia DR3 membership method finds more member stars in 21 rich open clusters than previous catalogs, and Bayesian isochrone fits yield age, metallicity, distance, and reddening posteriors.