tokens: The research leading to the presented results has received funding from the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no 338251 (StellarAges). E.B. undertook this research in the context of the International Max Planck Research School for Solar System Research. S.B. acknowledges partial support from NSF grant AST-1514676 and NASA grant NNX13AE70G. We thank Alexy Mints and the anonymous referee for their useful comments and discussions, which helped improve this manuscript. Software: Stellar models were calculated with Modules for Experiments in Stellar Astrophysics r8118 (MESA, Paxton et al. 2011 ) and stellar oscillations with the ADIPLS pulsation package 0.2 (Christensen-Dalsgaard 2008 ). Analysis in this manuscript was performed with python 3.5.1 libraries scikit-learn 0.17.1 (Pedregosa et al. 2011 ), NumPy 1.11.0 (Van Der Walt et al. 2011 ), matplotlib 1.5.1 (Hunter 2007 ), biokit 0.3.2 16 16 T. Cokelaer et al. 2016, (Version 0.3.2), https://github.com/biokit/biokit , and pandas 0.19.0 (McKinney 2010 ) as well as R 3.3.2 (R Core Team 2014 ) and the R libraries magicaxis 2.0.0 (Robotham 2015 ), RColorBrewer 1.1-2 (Neuwirth 2014 ), parallelMap 1.3 (Bischl Lang 2015 ), data.table 1.9.6 (Dowle et al. 2015 ), ggplot2 2.1.0 (Wickham 2009 ), GGally 1.2.0 (Schloerke et al. 2014 ), scales 0.4.0 (Wickham 2015 ) and Corrplot 0.77.
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