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Table 1.
Schema for the Clusters table.
| Column name | Units | Description | Data type |
|---|---|---|---|
| Cluster | – | Cluster name as used in Cantat-Gaudin et al. (2020). | str |
| Cluster_Simbad | – | Designation understandable by the Simbad (CDS) database. | str |
| ra_icrs | deg | RA of cluster centre in decimal degrees in ICRS, as given in Cantat-Gaudin et al. (2020). | float |
| dec_icrs | deg | Declination of cluster centre in decimal degrees in ICRS, as given in Cantat-Gaudin et al. (2020). | float |
| X | kpc | X coordinate in the Galactocentric coordinate system. Sun is at ( − 8.122, 0.0, 0.0208) kpc. | float |
| Y | kpc | X coordinate in the Galactocentric coordinate system. Sun is at ( − 8.122, 0.0, 0.0208) kpc. | float |
| Z | kpc | X coordinate in the Galactocentric coordinate system. Sun is at ( − 8.122, 0.0, 0.0208) kpc. | float |
| pmra | mas yr−1 | Proper motion in RA of cluster centre multiplied by cos(δ), as given in Cantat-Gaudin et al. (2020). | float |
| pmdec | mas yr−1 | Proper motion in declination of cluster centre, as given in Cantat-Gaudin et al. (2020). | float |
| parallax | mas | Parallax of cluster centre as given in Cantat-Gaudin et al. (2020). | float |
| radial_velocity | km s−1 | Radial velocity of cluster centre from Simbad. | float |
| radial_velocity_source | – | Source of radial velocity. | str |
| age | Myr | Age of the cluster from Cantat-Gaudin et al. (2020). | float |
| n | – | Number of stars calculated as the sum of all membership probabilities. | float |
| n_members | – | Number of stars with reported membership probability. | int |
| n_members_50 | – | Number of stars with membership probability > 0.5. | int |
| n_members_90 | – | Number of stars with membership probability > 0.9. | int |
| galaxia_com | – | Mean completeness (NGaia/NGalaxia) in the region of the cluster. | float |
| A_G | mag | Mean extinction in G band for stars with membership probability > 0.5 calculated using extinctions in Gaia DR3. | float |
| mass_func_index | – | Index of the power law of the mass function (α). | float |
| mass_func_charm | M⊙ | Characteristic mass of the mass function (mc). | float |
| mass_func_taper | – | Tapering exponent of the mass function (β). | float |
| mass_segregation | – | Mass segregation index calculated as max(Λ)/min(Λ). Large values indicate that mass segregation was detected. | float |
| cusp_index | – | Index describing the shape of the cluster. Small value indicates a distinct core, large value indicates a gradual decrease in density from the core to the tails. | float |
| tail_len | kpc | Length of tidal tail between most extreme points with ≥10 stars per 25 pc. | float |
| asym_index | – | Asymmetry index calculated as the ratio of the number of stars on each side of the cluster core. | float |
| pa_d_axis | deg | Position angle of the major axis used to calculate projected positions d_axis in the Members table | float |
| radial_velocity_measured | km s−1 | Radial velocity of the cluster core measured by us. | float |
| radial_velocity_std | km s−1 | Standard deviation of the radial velocities of all stars used to measure radial_velocity_measured. | float |
Notes. The table lists all the analysed clusters.
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