Fig. 5.

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Multicomponent empirical specfit analysis, including the AD model fitting result in the Hβ region after subtracting the continuum from the best fit. The upper abscissa is the rest-frame wavelength in Å and the lower abscissa is in radial velocity units. The vertical scale corresponds to the specific flux in units of 10−15 ergs s−1 cm−2 Å−1. The emission line components used in the fit are FeII (green), the broad AD model representing the fit for the broad double-peaked profile (red line), SBC (orange), and NC (blue). The black continuous line corresponds to the rest-frame spectrum. The dashed magenta line shows the final fitting from specfit. The dot-dashed vertical lines trace the rest-frame wavelength of Hβ. The lower panel shows the residual of the empirical fit.
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