Fig. A.2.
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Equivalent width of the Hδ absorption line and [OII] emission line at different positions in UVJ space. The two evolutionary tracks are of galaxies with 1 Gyr star formation duration but different quenching timescales, E(B-V)=0.15. Values in blue show the EW of [OII] emission lines, values in black the EW of Hδ absorption lines. A negative value represents absorption, and a positive value represents emission.
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