We have determined stellar membership based on astrometry, primarily from TGAS and HSOY, and multi-band photometry for 24 clusters within 333 pc. The fundamental cluster parameters (distance, age, and reddening) have been derived by fitting Padova isochrones (Bressan et al. 2012) to the cluster photometry using a chi-squared minimization.
Cone search capability for table J/A+A/615/A12/tablec (Membership lists for 24 clusters)
Cone search capability for table J/A+A/615/A12/table1 (List of derived parameters for 24 clusters)