Fig. 2.
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Age of the ALPINE galaxies as a function of sSFR assuming a Chabrier IMF (pink squares) and a THIMF (red circles). The cyan, orange, and green regions represent old (≳600 Myr), intermediate (300 − 600 Myr), and young (≲300 Myr) population of galaxies. The crossbars indicate the average error on the age and sSFR for the respective sample.
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