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Fig. 9

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Relative difference between the velocity dispersion measured from XSH and that measured from GAMA plotted against the σ measured from XSH. The fit was made on the ten objects in common within the same wavelength range and with the same fit settings. The disagreement is about 20% (shaded region) or more for galaxies with σ < 170 km s−1, and it is much smaller for galaxies with a higher velocity dispersion.

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