Fig. C.1

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Nucleosynthetic measurements for each of the isotopes considered in this work. Each panel represents a different element. The different meteorite classes are red to blue colored, and the horizontal error bars are the uncertainties on the nucleosynthetic composition. The corresponding estimates for their accretion ages are given with vertical error bars (or upper limit arrows). The upper axis represents the normalized values, similar to Fig. 8. The normalization is discussed in the text. The contours show the evolution of the mass fraction of unprocessed pebbles with time at different locations in the disk. The bold black line represents the inner disk composition at 1AU.
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