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Fig. 2


Comparison between the parameters derived by our method and those from the SEGUE Stellar Parameter Pipeline (SSPP) for 61,040 F- and G-type stars in DR8. Lefthand panels: density distribution of stars in a logarithmic scale, with the one-to-one relationship shown in yellow. Righthand panels: distribution of differences between this work and the SEGUE SSPP for each parameter, with Gaussian fittings and their central values in red.

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