Fig. 8
Some examples of the line-profiles comparison for the SDSS galaxies for which the BP fit error is smaller than 10%. The Hα (solid line), Hβ (dotted line), and Hγ (dashed line) broad components are shown. The name of the SDSS galaxy and the BP error f are given. Lines are smoothed according to the spectral S/N ratio, normalized to unity, and converted to the velocity scale.
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