Table 6.
Main properties of the BGG sample.
| BGG | g − r | (M/L)g |  |
fh, T |  |
Re | Rtr/Re | μtr | (g − r)R < Rtr | (g − r)R > Rtr |
|---|---|---|---|---|---|---|---|---|---|---|
| (mag) | (× 1011 M⊙) | (× 1011 M⊙) | (kpc) | (mag arcsec−2) | (mag) | (mag) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| NGC 5018 | 0.70 ± 0.20 | 1.97 | 2.9 | 92% | 2.7 | 6.37 | 5.37 | 26.6 | 0.78 | 0.94 |
| NGC 1533 | 0.77 ± 0.05 | 3.92 | 1.17 | 78% | 0.91 | 6.35 | 2.80 | 27.2 | 0.77 ± 0.04 | 0.49 ± 0.29 |
| IC 1459 | 0.84 ± 0.31 | 5.70 | 10.08 | 87% | 8.77 | 24.47 | 1.05 | 25.1 | 0.89 ± 0.29 | 0.44 ± 0.11 |
Notes. Column 1: BGG name. Column 2: averaged extinction-corrected g − r colour value. Column 3: mass-to-light ratio in g band. Column 4: total stellar mass. Columns 5 and 6: total accreted stellar mass fraction from the multi-component fit in g band and value in solar masses. Column 7: effective radius in g band. Columns 8 and 9: transition radius normalised to the effective radius and corresponding surface brightness. Columns 10 and 11: averaged extinction-corrected g − r colour value inside and outside the transition radius.
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