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Table 2.

Photometric properties of our nuclei from early-type hosts.

FDS ID FCC log10(M*, galaxy/M) log10(M*, nuc/M) (g′−r′)nuc [mag] (g′−i′)nuc [mag] fnuc/ftotal
(1) (2) (3) (4) (5) (6) (7)
FDS14_0133 FCC088 10.72 8.22 1.29 1.69 0.003
FDS11_0001 FCC184 10.66 8.33 1.53 2.31 0.005
FDS25_0000 FCC029 10.63 8.45 1.41 2.02 0.007
FDS11_0004 FCC170 10.23 8.07 1.91 2.27 0.007
FDS15_0002 FCC153 9.97 8.06 0.50 0.98 0.012
FDS7_0737 FCC310 9.78 7.67 1.19 1.55 0.008
FDS20_0000 FCC047 9.75 7.92 0.94 1.17 0.015
FDS16_0000 FCC148 9.68 7.78 0.33 0.65 0.013
FDS12_0002 FCC176 9.68 7.28 1.04 1.18 0.004
FDS11_0005 FCC190 9.66 7.18 1.02 1.13 0.003
... ... ... ... ... ... ...

Notes. We denote the host galaxy FDS identification number (1) and FCC designation (2) for each nucleus. From the multi-component decomposition models, we determine the galaxy and nucleus stellar masses (3) and (4), as well as the nucleus g′−r′ (5) and g′−i′ (6) colours. We also include the r′ band nucleus flux fraction (i.e. the fraction of light from the nucleus component compared to the total galaxy light; (7). Here, only an excerpt is shown; the full table can be found at the CDS.

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