Table C.1.
Quality cuts.
| Stetson photometry | Gaia photometry | Cluster parameters |
|---|---|---|
| χPSF < 4 | ipd_frac_multi_peak < 10 | E(B − V) < 1 |
| |sharp|< 1 | C*/σC* < 3 | [Fe/H] < −0.9 |
| I < 18 | Nstars, cl > 100 | |
| Nstars, distance > 2 | ||
| Membership probability > 0.5 |
Notes. The parameters χPSF and sharp were defined in Stetson et al. (2019). The definition of ipd_frac_multi_peak is given in the Gaia archive documentation, and that of the C* parameter was given in Riello et al. (2021). The E(B − V) and [Fe/H] values were taken from Harris (2010). The quantity Nstars, cl represents the total number of cluster members used by Cruz Reyes et al. (2024) to determine the cluster parameters, while Nstars, distance represents the number of stars used by Lengen et al. (2026) to determine the cluster distance via the Leavitt law. The membership probabilities were taken from Vasiliev & Baumgardt (2021).
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