Fig. 4
EW averaged in annuli for all 51 sources. Only the good signal/noise part of the cube that was used to fit the EW profile is shown. Diluted sources are drawn in purple, undiluted in orange and sources where the intrinsic value could not be determined due to the limited field of view of the SINFONI data are shown in green. The black line denotes NGC 5135 which has a non-axisymmetric EW profile. This graph shows sources observed in all three SINFONI pixel scales (field of view: 0.8, 3 and 8 arcsec).
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