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Fig. 13.
Star formation rate vs. the SSPs ages obtained with STECKMAP for CONT (top panels) and TAU1 (bottom panels) models with S/N = 10 (left column), and 50 (right column) at a galaxy age of 4.4 (top row), 180 (middle row), and 320 (bottom row) Myr. The vertical lines are indicated as in Fig. 5.
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