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In 2004, Balaguer-Núñez et al. re-evaluated the membership probabilities of 810 stars in the area of NGC 1817 open cluster, using both parametric and non-parametric approach. They have obtained absolute proper motions from 25 plates with maximum epoch difference of 81 years. Original results may be retrieved from corresponding article (Balaguer-Núñez et al., 2004 ), re-evulation by Clusterix system may be done by evaluating the data carried by following NGC 1817 cluster entity. No magnitudes are available, assigned values are therefore random and should not be taken into account when interpreting the results.
|Cluster name||Right ascension||Declination||Radius (arcmin)||Evaluate|
|NGC 1817||5h 12m 12.0s||16° 40' 58.8"||20.0||evaluate|