All Tables

Table 1: Log-book of the observations from FLAMES commissioning data archives: Palomar 13 observations and corresponding calibrations collected in HR-9 setup (514.3-535.4 nm). SNR is the average signal-to-noise ratio for star of V- ${\rm magnitude}=18$ .
Table 2: Barycentric radial velocities for 46 stars in the field centered on Palomar 13. The extra horizontal line isolates a clump of 11 stars with radial velocities very close to the systemic radial velocity of the star cluster, potentially members of the cluster.
Table 3: Membership probabilities from proper motions and positions in the CMD for the 11 stars with radial velocities implying membership of Palomar 13.