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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