Fig. 6.
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FWHM of the full profile of [O III]λλ4959,5007 versus centroid at 1/2 flux intensity (c(1/2)) for the [O III]λλ4959,5007 emission line. Blue and red squares indicate high-redshift sources from M09. Dashed line represents a linear regression. Colour scheme is the same as in Fig. 4. Error bars refer to 1σ level of confidence and were estimated only for our sample.
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