Fig. 9.
Comparison of stellar masses (in solar units), radii (in solar units), and ages (in Gyr) determined via stellar modeling using BASTA against those from stellar modeling using SPI. The biases in the residuals are all consistent with zero (0.001 ± 0.061 M⊙, −0.001 ± 0.027 R⊙, and −0.1 ± 1.0 Gyr).
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