Fig. 15
Same format as Fig. 14, only that the data are now binned in guiding-center radius, Rguide, rather than Galactocentric distance, to mitigate the effect of stellar mixing by “blurring”. Again, the colour-code represents the age, while the size and transparency now encode the uncertainty in stellar age and guiding-center radius. (If a star has a highly uncertain guiding radius – i.e. an Rguide PDF which extends over multiple R bins – it will appear as a faint dot in multiple panels of this figure.)
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