Table 1.
Open in new tab

Details of additional stars in table 2 of Hughes et al. (2022) with published [Fe/H] values from high dispersion spectroscopy.

Gaia DR3 SourceGALAH DR3 IDOther ID[Fe/H]Reference
3824738543969555840160421002101189HE 0926–0508−2.78Barklem et al. (2005)
6041027705498286464160415004601352SMSS J155730.10–293922.6−2.77Yong et al. (2021)
6403844758583266684170711005101182SMSS J213402.81–622421.1−3.12Yong et al. (2021)
Gaia DR3 SourceGALAH DR3 IDOther ID[Fe/H]Reference
3824738543969555840160421002101189HE 0926–0508−2.78Barklem et al. (2005)
6041027705498286464160415004601352SMSS J155730.10–293922.6−2.77Yong et al. (2021)
6403844758583266684170711005101182SMSS J213402.81–622421.1−3.12Yong et al. (2021)
Table 1.
Open in new tab

Details of additional stars in table 2 of Hughes et al. (2022) with published [Fe/H] values from high dispersion spectroscopy.

Gaia DR3 SourceGALAH DR3 IDOther ID[Fe/H]Reference
3824738543969555840160421002101189HE 0926–0508−2.78Barklem et al. (2005)
6041027705498286464160415004601352SMSS J155730.10–293922.6−2.77Yong et al. (2021)
6403844758583266684170711005101182SMSS J213402.81–622421.1−3.12Yong et al. (2021)
Gaia DR3 SourceGALAH DR3 IDOther ID[Fe/H]Reference
3824738543969555840160421002101189HE 0926–0508−2.78Barklem et al. (2005)
6041027705498286464160415004601352SMSS J155730.10–293922.6−2.77Yong et al. (2021)
6403844758583266684170711005101182SMSS J213402.81–622421.1−3.12Yong et al. (2021)
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