Fig. 1
Schematic overplot of the NIFS (red) and GMOS (blue) field-of-view on the WFPC2 F606 image. The kinematic data only map the very core of NGC 4414 which is not polluted by dust. The orientation of the NIFS data is 150° and that of the GMOS data is 60° counterclockwise from north. The star in the south-western part of the bulge served as a natural guide star for our observations.
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