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Fig. 3.

image

Residual image of FCC 47 after subtracting a MGE model of the galaxy. The coloured crosses show the position of GC candidates in the HST catalogue of Jordán et al. (2015), colour-coded by their g-band magnitude. The black circles show the position of 42 GC candidates that are found with the DAOSTARFINDER routine in the MUSE data by cross referencing with the catalogue. The diamond indicates the position of FCC 47-UCD1 with a g-band magnitude of ∼21 mag. The triangles indicate the positions of emission-line background galaxies we found in the MUSE cube.

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