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Fig. 1.

image

Six galaxies of the main SFvirialized sample. The panels show for each galaxy the extracted spectrum (black solid line) over an area of 25 spaxels with the fitted Gaussians by KUBEVIZ to Hα and [N II] λ 6584 shown in green and the noise spectrum as a solid red line. It can be seen that the measurements of Hα and [N II] λ 6584 are not affected by strong sky lines (peaks of the solid red lines).

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