Fig. 7
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Distribution of ages in the full GALAH DR3 sample (light grey histogram) and sources that match the UVW and metallicity of LP 890-9 to within 10 km s−1 and 1σ, respectively (dark grey histogram). The latter has a broad peak at 
Gyr (yellow line with uncertainties indicated by the green shaded region), which we take as an estimate for the age of LP 890-9.
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