Correlated accretion ages and ε54Cr of meteorite parent bodies and the evolution of the solar nebula

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The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “Chondrite parent bodies generally accreted later, with most OCs probably accreting 9 CI 3.6 ± 0.5a 4.4 − 5.7aa 3.1 - 4.1 a. Sugiura & Fujiya (2014); b. Melting event, Al-Mg: Baker et al. (2012); c. Impact event, Al-Mg and Hf-W: van Kooten et al. (2017); d. Wilson & Goodrich (2016); Goodrich et al.…”
The Non-carbonaceous–Carbonaceous Meteorite Dichotomy (2020, background): “Recent summaries of accretion ages can be found in Sugiura and Fujiya (2014), Desch et al. (2018), and Kruijer et al. (2020).”
The Compositional Structure of the Asteroid Belt (2015, background): “The average ages and estimates of the accretion ages of chondrites and various non-chondrites from Sugiura and Fujiya (2014) unless otherwise indicated.”