Fig. 2
Spatially integrated rest frame spectra from the nucleus of each galaxy in the H band. The spatial area used in the integration is shown in Figs. 4 and 5 by a black rectangle. Each spectrum is integrated over an 8 × 8 pixel area. The FeII1.64 emission line is denoted by a dashed line and marked along the top of the figure. Several spectra are degraded by residual atmospheric OH features.
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