Table 6.
Parameters of LTGs with disc-breaks.
| Object | Br | σnBr | μBr | hin | hout | Hubble | Break | |||
|---|---|---|---|---|---|---|---|---|---|---|
| [arcsec] | [kpc] | [arcsec] | [ ] |
[arcsec] | g − i [mag] | [arcsec] | g − i [mag] | Type (T) | Type | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |||
| FCC113 | – | – | – | – | – | – | – | – | 6 | I |
| FCC115 | 15.35 | 1.47 | 1.07 | 23.52 | 6.84 | 0.25 ± 0.03 | 16.15 | 0.12 ± 0.03 | 8 | II |
| FCC121 | 192.35 | 18.46 | 7.05 | 23.65 | 63.9 | 0.88 ± 0.02 | 175.7 | 1.09 ± 0.04 | 3 | III+II |
| FCC176 | 38.86 | 3.73 | 6.39 | 22.20 | 28.66 | 1.10 ± 0.02 | 54.73 | 0.76 ± 0.2 | 1 | II |
| FCC179 | 73.02 | 7.01 | 3.66 | 21.98 | 43.47 | 1.10 ± 0.02 | 50.08 | 1.05 ± 0.02 | 1 | II |
| FCC263 | 24.12 | 2.32 | 1.58 | 22.06 | 14.42 | 0.49 ± 0.02 | 37.39 | 0.63 ± 0.02 | 2 | III |
| FCC267 | 14.95 | 1.43 | 0.39 | 23.83 | 8.52 | 0.76 ± 0.03 | 22.11 | 1.26 ± 0.13 | 9 | III |
| FCC285 | – | – | – | – | – | – | – | – | 7 | I |
| FCC290 | 47.31 | 4.54 | 3.42 | 21.45 | 23.22 | 0.72 ± 0.03 | 70.66 | 0.71± 0.02 | 4 | II |
| FCC302 | – | – | – | – | – | – | – | – | 8 | I |
| FCC306 | 6.88 | 0.66 | 0.15 | 21.81 | 2.92 | 0.09 ± 0.01 | 14.1 | −0.39 ± 0.07 | 9 | II |
| FCC308 | 25.60 | 2.46 | 0.84 | 22.32 | 14.11 | 0.71 ± 0.02 | 92.25 | 0.75 ± 0.04 | 7 | III |
| FCC312 | 72.06 | 6.91 | 2.93 | 23.38 | 42.17 | 1.16 ± 0.05 | 67.79 | 1.54 ± 0.03 | 7 | III |
Notes. Column 1 – LTGs with a disc-break; Column 2 – Break radius in units of arcsec and kpc (1 arcsec = 0.096 kpc); Column 3 – Standard deviation of the break radii from (n + 1)3 combinations; Column 4 – Surface brightness at the break radius; Column 5 – inner scale-length in units of arcsec, and average (g − i) colour for hin; Column 6 – outer scale-length in units of arcsec, and average (g − i) colour for hout; Column 7– Hubble Type T ; Column 8 – Profile classification (FCC267 and FCC308 are also classified as Type III+II, but we do not mention them in Table 6 due to lack of data points to be fitted with the algorithm (see Sect. 4.2)).
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