Fig. 4.
Normalised Brγ profile from SINFONI (blue) with the best-fit line profile model (orange). The model is the combination of a narrow line template determined by the [O III]λ5007 Å line from X-shooter spectra (green) and a broad component consisting of two Gaussians (red). The residuals (purple) show that our fit very closely matches the observed Brγ profile.
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