Table C1.
Open in new tab

Effective temperature, gravity, and abundances for 19 elements in eight NGC 1901 stars.

Gaia DR2 source idTeff Klog g dex|$\left[\frac{\mathrm{Li}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{C}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{O}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Na}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mg}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Al}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Si}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{K}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ca}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Sc}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ti}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cr}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Fe}}{\mathrm{H}} \right]$| dex|$\left[\frac{\mathrm{Ni}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cu}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Zn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Y}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ba}}{\mathrm{Fe}} \right]$| dex
465851570046524339262654.170.030.040.090.140.130.18–0.05–0.12–0.29–0.110.47
465872752823270297664834.040.070.21–0.020.020.210.140.100.120.050.06–0.05–0.29–0.060.150.44
465876611422117504058404.401.850.06–0.02–0.050.110.03–0.15–0.110.100.050.94
465833853731357209659824.351.88–0.03–0.070.030.110.12–0.100.05–0.16–0.090.070.44
465874360859078643260764.291.770.180.010.100.030.090.050.100.020.03–0.03–0.29–0.13–0.050.060.60
465876611422117504065964.120.080.040.090.110.230.17–0.270.010.56
465873226555542195260084.342.140.09–0.060.02–0.130.030.110.090.08–0.010.12–0.07–0.190.00–0.060.050.280.48
465854833788195942460154.250.540.160.080.240.160.18–0.450.040.79
Gaia DR2 source idTeff Klog g dex|$\left[\frac{\mathrm{Li}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{C}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{O}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Na}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mg}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Al}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Si}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{K}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ca}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Sc}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ti}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cr}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Fe}}{\mathrm{H}} \right]$| dex|$\left[\frac{\mathrm{Ni}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cu}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Zn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Y}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ba}}{\mathrm{Fe}} \right]$| dex
465851570046524339262654.170.030.040.090.140.130.18–0.05–0.12–0.29–0.110.47
465872752823270297664834.040.070.21–0.020.020.210.140.100.120.050.06–0.05–0.29–0.060.150.44
465876611422117504058404.401.850.06–0.02–0.050.110.03–0.15–0.110.100.050.94
465833853731357209659824.351.88–0.03–0.070.030.110.12–0.100.05–0.16–0.090.070.44
465874360859078643260764.291.770.180.010.100.030.090.050.100.020.03–0.03–0.29–0.13–0.050.060.60
465876611422117504065964.120.080.040.090.110.230.17–0.270.010.56
465873226555542195260084.342.140.09–0.060.02–0.130.030.110.090.08–0.010.12–0.07–0.190.00–0.060.050.280.48
465854833788195942460154.250.540.160.080.240.160.18–0.450.040.79
Table C1.
Open in new tab

Effective temperature, gravity, and abundances for 19 elements in eight NGC 1901 stars.

Gaia DR2 source idTeff Klog g dex|$\left[\frac{\mathrm{Li}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{C}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{O}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Na}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mg}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Al}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Si}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{K}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ca}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Sc}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ti}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cr}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Fe}}{\mathrm{H}} \right]$| dex|$\left[\frac{\mathrm{Ni}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cu}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Zn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Y}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ba}}{\mathrm{Fe}} \right]$| dex
465851570046524339262654.170.030.040.090.140.130.18–0.05–0.12–0.29–0.110.47
465872752823270297664834.040.070.21–0.020.020.210.140.100.120.050.06–0.05–0.29–0.060.150.44
465876611422117504058404.401.850.06–0.02–0.050.110.03–0.15–0.110.100.050.94
465833853731357209659824.351.88–0.03–0.070.030.110.12–0.100.05–0.16–0.090.070.44
465874360859078643260764.291.770.180.010.100.030.090.050.100.020.03–0.03–0.29–0.13–0.050.060.60
465876611422117504065964.120.080.040.090.110.230.17–0.270.010.56
465873226555542195260084.342.140.09–0.060.02–0.130.030.110.090.08–0.010.12–0.07–0.190.00–0.060.050.280.48
465854833788195942460154.250.540.160.080.240.160.18–0.450.040.79
Gaia DR2 source idTeff Klog g dex|$\left[\frac{\mathrm{Li}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{C}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{O}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Na}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mg}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Al}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Si}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{K}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ca}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Sc}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ti}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cr}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Mn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Fe}}{\mathrm{H}} \right]$| dex|$\left[\frac{\mathrm{Ni}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Cu}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Zn}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Y}}{\mathrm{Fe}} \right]$| dex|$\left[\frac{\mathrm{Ba}}{\mathrm{Fe}} \right]$| dex
465851570046524339262654.170.030.040.090.140.130.18–0.05–0.12–0.29–0.110.47
465872752823270297664834.040.070.21–0.020.020.210.140.100.120.050.06–0.05–0.29–0.060.150.44
465876611422117504058404.401.850.06–0.02–0.050.110.03–0.15–0.110.100.050.94
465833853731357209659824.351.88–0.03–0.070.030.110.12–0.100.05–0.16–0.090.070.44
465874360859078643260764.291.770.180.010.100.030.090.050.100.020.03–0.03–0.29–0.13–0.050.060.60
465876611422117504065964.120.080.040.090.110.230.17–0.270.010.56
465873226555542195260084.342.140.09–0.060.02–0.130.030.110.090.08–0.010.12–0.07–0.190.00–0.060.050.280.48
465854833788195942460154.250.540.160.080.240.160.18–0.450.040.79
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