Fig. A.1.
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Specific star formation rate distribution in stellar mass bins, compared to SDSS DR8 observational estimates (grey shaded histograms). The MS and MSII histograms have been slightly shifted (by 0.05 dex) for clarity. The black solid, black dashed, and red solid lines refer the GAEA model version presented in DL24 and run on MS, MSII, and PMS, respectively.
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