Fig. 7.

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Single Gaussian (1G) and double Gaussian (2G, narrow + broad) best fits to the [O III] λ5007 Å+Hβ and Hα lines, as indicated in each panel label, for the two galaxies (ID GLASS 160133 and 110000) in which we detect a significant outflow signature in both emission lines (upper and lower four panels, respectively). In each panel, the upper part shows the observed spectrum with the best fit line in red (red (green) line for the narrow (broad) component in the double Gaussian fit), the middle part represents the error spectrum, while the bottom part is the residual after subtracting the best fit result. The spectra are in the observed frame wavelength.
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