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The Interstellar Medium in [O III] selected Star forming Galaxies at z similar to 3 2

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Figure

Figure 1.Redshift distribution of the spectroscopicallyshown. The wavelength range of the NBto the redshift ranges for the [sources
Figure 2.SFRtroscopically confirmed galaxies.the extra extinction to the nebular emission, i.e
Figure 4.Stacked spectra of the [Oiii] emitters obtained by dividing the samples into two stellar mass bins of 9.76 ≤log(M∗/M⊙) ≤ 10.21 and 9.07 ≤ log(M∗/M⊙) ≤ 9.23
Figure 6.Relations between four line ratios and metallicities calibrated with the Curti et al
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