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Table 1

Data on the stellar sample taken from the Hypatia Database.

# HIP Fe C O Mg Si S SpTy d (pc) Teff (K)
0 Sun 7.5 ± 0.04 8.43 ± 0.05 8.69 ± 0.05 7.60 ± 0.04 7.51 ± 0.03 7.12 ± 0.03 G2V 0 5778

1 109836 +0.39 +0.225 +0.25 +0.15 +0.285 +0.277 G6V 72.8 5810
2 28869 +0.13 +0.01 +0.02 −0.09 +0.17 +0.12 G0V 47.8 6120
3 63048 −0.019 +0.13 +0.19 +0.25 +0.08 +0.23 G2V 43.05 5665
4 43393 −0.57 −0.305 +0.03 −0.293 −0.329 +0.1 G8/K0V 49.67 5306
5 99423 −1.335 −0.49 −0.265 −0.93 −0.92 +0.21 G0V 109.58 5745

6 83359 +0.145 −0.15 −0.03 +0.1 +0.46 +1.1 G5-K1III 110.63 4949

Notes. The full set of chemical abundances used for each star can be seen in Appendix A. The red value indicates an elemental abundance that is not available in the Hypatia Database but is inferred from the median of the known data for the metals of the specific star. Star 0 represents the Sun and is the reference to which any comparison is made. Stars 1–5 are main sequence G-type stars. Star 6 is separated from the rest since it is a red giant; its spectral type (SpTy) and effective temperature (Teff) are from Liu et al. (2010).

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