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Table 3

Elemental abundances of NGC 6569 members.

Apogee ID S/N [C/Fe] [N/Fe] [O/Fe] [Mg/Fe] [A1/Fe] [Si/Fe] [Ca/Fe] [Ti/Fe] [Fe/H] [Ni/Fe] [Ce/Fe] [Nd/Fe]
2M18132448-3149140 276 −0.05 +0.51 +0.34 +0.44 +0.28 +0.20 +0.22 +0.39 −0.83 +0.04 +0.26 +0.41
2M18133940-3150132 222 −0.56 +0.99 +0.16 +0.46 +0.78 +0.32 +0.33 +0.56 −0.87 +0.07 +0.43 +0.51
2M18134025-3149477 174 −0.11 +0.34 +0.32 +0.34 +0.21 +0.39 +0.15 +0.13 −0.96 −0.01 +0.19 +0.48
2M18133789-3147295 171 −0.48 +1.09 +0.30 +0.54 +0.41 +0.38 +0.17 +0.13 −0.93 +0.07 +0.35 +0.49
2M18133324-3150194 153 −0.29 +1.24 +0.38 +0.49 +0.49 +0.36 +0.35 +0.43 −0.92 +0.10 +0.32 +0.46
2M18133083-3148103 130 −0.26 +0.90 +0.26 +0.39 +0.40 +0.42 +0.10 +0.55 −0.90 −0.10 +0.34 +0.25
2M18133620-3149040 136 −0.11 +0.28 +0.39 +0.41 +0.21 +0.28 +0.39 +0.37 −0.83 +0.00 +0.23 +0.47
2M18134151-3148556 119 −0.12 +0.53 +0.49 +0.34 +0.21 +0.37 +0.38 +0.17 −0.99 +0.04 +0.24 +0.51
2M18134725-3147570 64 +0.40 +0.37 +0.38 +0.35 +0.62 −0.90 +0.10
2M18135154-3151406 60 −0.02 +0.41 +0.68 +0.58 +0.35 +0.26 +0.40 +0.37 −0.85 +0.10 +0.18 +0.46
2M18133329-3146211 51 +0.29 +0.22 +0.31 +0.30 −1.02 −0.04
Mean −0.22 +0.68 +0.39 +0.43 +0.35 +0.35 +0.28 +0.37 −0.91 +0.03 +0.28 +0.45
Std +0.18 +0.34 +0.15 +0.08 +0.17 +0.07 +0.10 +0.18 +0.06 +0.06 +0.08 +0.08
ASPCAP DR17
Mean −0.21 +0.66 +0.30 +0.32 +0.33 +0.29 +0.28 +0.12 −0.96 +0.04 +0.12
Std +0.16 +0.45 +0.07 +0.04 +0.20 +0.06 +0.12 +0.16 +0.07 +0.03 +0.25
Spec(Uncalibrated)
Mean −0.23 +0.74 +0.32 +0.39 +0.41 +0.40 +0.29 +0.19 −0.95 +0.03 +0.20 +0.36
Std +0.10 +0.52 +0.07 +0.12 +0.22 +0.13 +0.10 +0.15 +0.08 +0.06 +0.11 +0.08
Spec(Calibrated)
Mean −0.13 +0.95 +0.48 +0.48 +0.53 +0.55 +0.37 +0.39 −0.91 +0.03 +0.36 +0.48
Std +0.09 +0.50 +0.11 +0.06 +0.17 +0.11 +0.09 +0.09 +0.06 +0.10 +0.12 +0.10
Johnson et al. (2018)
Mean +0.38 +0.41 +0.52 +0.35 +0.21 −0.87 −0.08
Std +0.31 +0.09 +0.14 +0.09 +0.10 +0.06 +0.05
Valenti et al. (2011)
Mean −0.27 +0.48 +0.50 +0.38 +0.49 +0.31 +0.40 −0.79
Std +0.11 +0.09 +0.06 +0.11 +0.08 +0.04 +0.04 +0.05

Notes. For each species, we show the mean value and the standard deviation. We compare with values estimated with ASPCAP/APOGEE DR17 and with previous high-resolution studies on this cluster Johnson et al. (2018) and Valenti et al. (2011). The Solar reference abundances are from Asplund et al. (2005), except for Ce and Nd, which is taken from Grevesse et al. (2015).

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