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Fig. 10

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NLTE corrections for Fe I in all metal-poor SAGA stars as a function of their [Fe I/H]LTE, using the mean corrections from Mashonkina et al. (2011) and Bergemann et al. (2012c). The data points are colour-coded by log g. The circles represent stars whose parameters fall within the grid and the star symbols mark those outside the grid boundaries.

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