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Fig. 1


Probability distribution function for log(age) (top row), mass (middle row), and distance modulus (bottom row) for two stars from our catalogue. Different evolutionary stages are indicated with different colours (see legend). The stages are main-sequence stars and giants ascending the red giant branch (pre-core-helium burning, stage I), core-helium burning stars (stage II) and asymptotic giant branch stars (post-core-helium burning, stage III). The histograms represent model distributions and solid lines indicate our fits for individual USPDFs.

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