Table 1.

SMC star cluster properties.

IDdRef.[Fe/H]Ref.
(kpc)(dex)
AM362.8 ± 4.61−0.75 ± 0.114
B99 –−0.84 ± 0.045
B16861.9 ± 2.12−1.08 ± 0.0910
BS121 –−0.66 ± 0.076
BS18852.7 ± 3.02−0.94 ± 0.1310
BS19650.1 ± 2.02−0.89 ± 0.0810
H86-97 –−0.71 ± 0.055
HW31 –−1.12 ± 0.378
HW4065.5 ± 4.21−0.78 ± 0.055
HW41 –−0.96 ± 0.368
HW4254.5 ± 2.73−0.95 ± 0.428
HW47 –−0.92 ± 0.046
HW5653.5 ± 1.22−0.97 ± 0.2010
HW67 –−0.72 ± 0.045
HW84 –−0.91 ± 0.056
HW8554.0 ± 1.62−0.82 ± 0.1410
HW86 –−0.61 ± 0.066
IC170865.2 ± 1.52−1.11 ± 0.1710
K360.6 ± 1.12−0.85 ± 0.035
K6 –−0.63 ± 0.025
K764.3 ± 2.44−0.83 ± 0.067
K869.8 ± 2.32−0.76 ± 0.074
K9 –−1.12 ± 0.055
K3762.4 ± 2.04−0.79 ± 0.115
K3866.7 ± 1.94−0.65 ± 0.188
K4462.2 ± 2.72−0.78 ± 0.037
L156.9 ± 1.02−1.04 ± 0.035
L254.5 ± 3.51−1.28 ± 0.094
L353.5 ± 3.41−0.75 ± 0.338
L453.7 ± 2.42−1.08 ± 0.046
L5 –−1.25 ± 0.056
L654.9 ± 2.32−1.24 ± 0.036
L7 –−0.76 ± 0.066
L19 –−0.87 ± 0.036
L27 –−1.14 ± 0.066
L32 –−0.96 ± 0.047
L3864.0 ± 1.11−1.39 ± 0.037
L4358.8 ± 3.34−0.94 ± 0.037
L91 –−1.01 ± 0.358
L10058.6 ± 0.72−0.89 ± 0.1410
L106 –−0.88 ± 0.066
L108 –−1.05 ± 0.056
L11047.9 ± 2.32−1.03 ± 0.056
L112 –−1.08 ± 0.075
L11350.5 ± 1.72−1.03 ± 0.045
L116 –−0.89 ± 0.027
NGC12164.9 ± 1.22−1.19 ± 0.129
NGC15261.9 ± 5.41−0.72 ± 0.027
NGC33957.6 ± 4.12−1.15 ± 0.027
NGC36155.8 ± 1.72−0.90 ± 0.037
NGC41151.8 ± 3.31−0.74 ± 0.047
NGC41660.0 ± 1.91−0.85 ± 0.047
NGC41956.2 ± 1.32−0.62 ± 0.027
NGC643 –−0.82 ± 0.036
OGLE-SMC113 –−0.80 ± 0.075
IDdRef.[Fe/H]Ref.
(kpc)(dex)
AM362.8 ± 4.61−0.75 ± 0.114
B99 –−0.84 ± 0.045
B16861.9 ± 2.12−1.08 ± 0.0910
BS121 –−0.66 ± 0.076
BS18852.7 ± 3.02−0.94 ± 0.1310
BS19650.1 ± 2.02−0.89 ± 0.0810
H86-97 –−0.71 ± 0.055
HW31 –−1.12 ± 0.378
HW4065.5 ± 4.21−0.78 ± 0.055
HW41 –−0.96 ± 0.368
HW4254.5 ± 2.73−0.95 ± 0.428
HW47 –−0.92 ± 0.046
HW5653.5 ± 1.22−0.97 ± 0.2010
HW67 –−0.72 ± 0.045
HW84 –−0.91 ± 0.056
HW8554.0 ± 1.62−0.82 ± 0.1410
HW86 –−0.61 ± 0.066
IC170865.2 ± 1.52−1.11 ± 0.1710
K360.6 ± 1.12−0.85 ± 0.035
K6 –−0.63 ± 0.025
K764.3 ± 2.44−0.83 ± 0.067
K869.8 ± 2.32−0.76 ± 0.074
K9 –−1.12 ± 0.055
K3762.4 ± 2.04−0.79 ± 0.115
K3866.7 ± 1.94−0.65 ± 0.188
K4462.2 ± 2.72−0.78 ± 0.037
L156.9 ± 1.02−1.04 ± 0.035
L254.5 ± 3.51−1.28 ± 0.094
L353.5 ± 3.41−0.75 ± 0.338
L453.7 ± 2.42−1.08 ± 0.046
L5 –−1.25 ± 0.056
L654.9 ± 2.32−1.24 ± 0.036
L7 –−0.76 ± 0.066
L19 –−0.87 ± 0.036
L27 –−1.14 ± 0.066
L32 –−0.96 ± 0.047
L3864.0 ± 1.11−1.39 ± 0.037
L4358.8 ± 3.34−0.94 ± 0.037
L91 –−1.01 ± 0.358
L10058.6 ± 0.72−0.89 ± 0.1410
L106 –−0.88 ± 0.066
L108 –−1.05 ± 0.056
L11047.9 ± 2.32−1.03 ± 0.056
L112 –−1.08 ± 0.075
L11350.5 ± 1.72−1.03 ± 0.045
L116 –−0.89 ± 0.027
NGC12164.9 ± 1.22−1.19 ± 0.129
NGC15261.9 ± 5.41−0.72 ± 0.027
NGC33957.6 ± 4.12−1.15 ± 0.027
NGC36155.8 ± 1.72−0.90 ± 0.037
NGC41151.8 ± 3.31−0.74 ± 0.047
NGC41660.0 ± 1.91−0.85 ± 0.047
NGC41956.2 ± 1.32−0.62 ± 0.027
NGC643 –−0.82 ± 0.036
OGLE-SMC113 –−0.80 ± 0.075

Note.(1) de Grijs & Bono (2015); (2) Piatti (2021a); (3) Piatti (2022); (4) Dias et al. (2022); (5) Parisi et al. (2015); (6) Parisi et al. (2009); (7) Parisi et al. (2022); (8) De Bortoli et al. (2022); (9) Da Costa & Hatzidimitriou (1998); (10) Dias et al. (2021).

Table 1.

SMC star cluster properties.

IDdRef.[Fe/H]Ref.
(kpc)(dex)
AM362.8 ± 4.61−0.75 ± 0.114
B99 –−0.84 ± 0.045
B16861.9 ± 2.12−1.08 ± 0.0910
BS121 –−0.66 ± 0.076
BS18852.7 ± 3.02−0.94 ± 0.1310
BS19650.1 ± 2.02−0.89 ± 0.0810
H86-97 –−0.71 ± 0.055
HW31 –−1.12 ± 0.378
HW4065.5 ± 4.21−0.78 ± 0.055
HW41 –−0.96 ± 0.368
HW4254.5 ± 2.73−0.95 ± 0.428
HW47 –−0.92 ± 0.046
HW5653.5 ± 1.22−0.97 ± 0.2010
HW67 –−0.72 ± 0.045
HW84 –−0.91 ± 0.056
HW8554.0 ± 1.62−0.82 ± 0.1410
HW86 –−0.61 ± 0.066
IC170865.2 ± 1.52−1.11 ± 0.1710
K360.6 ± 1.12−0.85 ± 0.035
K6 –−0.63 ± 0.025
K764.3 ± 2.44−0.83 ± 0.067
K869.8 ± 2.32−0.76 ± 0.074
K9 –−1.12 ± 0.055
K3762.4 ± 2.04−0.79 ± 0.115
K3866.7 ± 1.94−0.65 ± 0.188
K4462.2 ± 2.72−0.78 ± 0.037
L156.9 ± 1.02−1.04 ± 0.035
L254.5 ± 3.51−1.28 ± 0.094
L353.5 ± 3.41−0.75 ± 0.338
L453.7 ± 2.42−1.08 ± 0.046
L5 –−1.25 ± 0.056
L654.9 ± 2.32−1.24 ± 0.036
L7 –−0.76 ± 0.066
L19 –−0.87 ± 0.036
L27 –−1.14 ± 0.066
L32 –−0.96 ± 0.047
L3864.0 ± 1.11−1.39 ± 0.037
L4358.8 ± 3.34−0.94 ± 0.037
L91 –−1.01 ± 0.358
L10058.6 ± 0.72−0.89 ± 0.1410
L106 –−0.88 ± 0.066
L108 –−1.05 ± 0.056
L11047.9 ± 2.32−1.03 ± 0.056
L112 –−1.08 ± 0.075
L11350.5 ± 1.72−1.03 ± 0.045
L116 –−0.89 ± 0.027
NGC12164.9 ± 1.22−1.19 ± 0.129
NGC15261.9 ± 5.41−0.72 ± 0.027
NGC33957.6 ± 4.12−1.15 ± 0.027
NGC36155.8 ± 1.72−0.90 ± 0.037
NGC41151.8 ± 3.31−0.74 ± 0.047
NGC41660.0 ± 1.91−0.85 ± 0.047
NGC41956.2 ± 1.32−0.62 ± 0.027
NGC643 –−0.82 ± 0.036
OGLE-SMC113 –−0.80 ± 0.075
IDdRef.[Fe/H]Ref.
(kpc)(dex)
AM362.8 ± 4.61−0.75 ± 0.114
B99 –−0.84 ± 0.045
B16861.9 ± 2.12−1.08 ± 0.0910
BS121 –−0.66 ± 0.076
BS18852.7 ± 3.02−0.94 ± 0.1310
BS19650.1 ± 2.02−0.89 ± 0.0810
H86-97 –−0.71 ± 0.055
HW31 –−1.12 ± 0.378
HW4065.5 ± 4.21−0.78 ± 0.055
HW41 –−0.96 ± 0.368
HW4254.5 ± 2.73−0.95 ± 0.428
HW47 –−0.92 ± 0.046
HW5653.5 ± 1.22−0.97 ± 0.2010
HW67 –−0.72 ± 0.045
HW84 –−0.91 ± 0.056
HW8554.0 ± 1.62−0.82 ± 0.1410
HW86 –−0.61 ± 0.066
IC170865.2 ± 1.52−1.11 ± 0.1710
K360.6 ± 1.12−0.85 ± 0.035
K6 –−0.63 ± 0.025
K764.3 ± 2.44−0.83 ± 0.067
K869.8 ± 2.32−0.76 ± 0.074
K9 –−1.12 ± 0.055
K3762.4 ± 2.04−0.79 ± 0.115
K3866.7 ± 1.94−0.65 ± 0.188
K4462.2 ± 2.72−0.78 ± 0.037
L156.9 ± 1.02−1.04 ± 0.035
L254.5 ± 3.51−1.28 ± 0.094
L353.5 ± 3.41−0.75 ± 0.338
L453.7 ± 2.42−1.08 ± 0.046
L5 –−1.25 ± 0.056
L654.9 ± 2.32−1.24 ± 0.036
L7 –−0.76 ± 0.066
L19 –−0.87 ± 0.036
L27 –−1.14 ± 0.066
L32 –−0.96 ± 0.047
L3864.0 ± 1.11−1.39 ± 0.037
L4358.8 ± 3.34−0.94 ± 0.037
L91 –−1.01 ± 0.358
L10058.6 ± 0.72−0.89 ± 0.1410
L106 –−0.88 ± 0.066
L108 –−1.05 ± 0.056
L11047.9 ± 2.32−1.03 ± 0.056
L112 –−1.08 ± 0.075
L11350.5 ± 1.72−1.03 ± 0.045
L116 –−0.89 ± 0.027
NGC12164.9 ± 1.22−1.19 ± 0.129
NGC15261.9 ± 5.41−0.72 ± 0.027
NGC33957.6 ± 4.12−1.15 ± 0.027
NGC36155.8 ± 1.72−0.90 ± 0.037
NGC41151.8 ± 3.31−0.74 ± 0.047
NGC41660.0 ± 1.91−0.85 ± 0.047
NGC41956.2 ± 1.32−0.62 ± 0.027
NGC643 –−0.82 ± 0.036
OGLE-SMC113 –−0.80 ± 0.075

Note.(1) de Grijs & Bono (2015); (2) Piatti (2021a); (3) Piatti (2022); (4) Dias et al. (2022); (5) Parisi et al. (2015); (6) Parisi et al. (2009); (7) Parisi et al. (2022); (8) De Bortoli et al. (2022); (9) Da Costa & Hatzidimitriou (1998); (10) Dias et al. (2021).

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