Fig. 4.

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Positions of the globular cluster candidates with respect to the center of the galaxy. The plot shows declination and right ascension of the sources, in which the center of NGC 4696 is located at (Δα, Δδ) = (0, 0). The blue circles define the borders of the annulus inside of which the azimuthal distribution of the GCs was calculated, whereas the red rectangles represent the regions where the contamination level from background objects and foreground stars was calculated.
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