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Fig. 1


Evolutionary tracks for a 1 M model for various stellar evolution codes. The box represents the estimated post-Gaia uncertainties of the luminosity and effective temperature. Top: models comuputed with a metallicity of Z ≈ 0.02. The inset shows a zoomed in region around the solar luminosity and temperature, with the box displaying the uncertainties of the solar luminosity and effective temperature. Bottom: models computing using the abundances of Asplund et al. (2009). The Padova track, which is intermediate in metallicity is included in both panels.

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