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Fig. 18.

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Stellar mass, SFR, and Hα and [OIII]λ5007 attenuation. We compare the derived parameters using photometry and Hα flux in the SED fitting and adding Hβ and [OIII]λ5007 fluxes. The three different gas-phase metallicity bins are presented as blue circles, orange squares, and green triangles as in Fig. 17. The mean offset and dispersion of the are shown for each parameter.

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