Table 4.
Derived Parameters of LTGs inside Fornax cluster’s virial radius.
| Object | mu | mg | mr | mi | Reu | Reg | Rer | Rei |
|---|---|---|---|---|---|---|---|---|
| mag | mag | mag | mag | arcsec | arcsec | arcsec | arcsec | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| FCC113 | 15.51 ± 0.04 | 15.01 ± 0.02 | 14.44 ± 0.01 | 14.3 ± 0.01 | 29.74 ± 0.76 | 19.51 ± 0.19 | 20.56 ± 0.1 | 20.64 ± 0.108 |
| FCC115 | 17.18 ± 0.01 | 16.35 ± 0.01 | 15.91 ± 0.39 | 15.94 ± 0.01 | 17.9 ± 0.5 | 19.54 ± 0.11 | 20.58 ± 0.11 | 16.58 ± 0.2 |
| FCC121 | 10.65 ± 0.05 | 9.33 ± 0.04 | 8.79 ± 0.03 | 8.43 ± 0.03 | 134 ± 3.98 | 142.4 ± 3.69 | 109.8 ± 2.15 | 132.8 ± 2.89 |
| FCC176 | 13.95 ± 0.01 | 12.51 ± 0.01 | 11.74 ± 0.01 | 11.45 ± 0.01 | 56.76 ± 1.59 | 53.03 ± 0.69 | 53.73 ± 2.28 | 47.42 ± 1.20 |
| FCC179 | 13.17 ± 0.02 | 11.44 ± 0.01 | 10.68 ± 0.01 | 10.34 ± 0.01 | 22.75 ± 0.42 | 29.68 ± 0.50 | 30.03 ± 0.50 | 28.01 ± 0.73 |
| FCC263 | 14.72 ± 0.05 | 12.91 ± 0.05 | 12.7 ± 0.02 | 12.58 ± 0.01 | 21.82 ± 1.57 | 25.36 ± 1.67 | 27.15 ± 0.56 | 21.53 ± 0.14 |
| FCC267 | 16.6 ± 0.08 | 15.68 ± 0.03 | 15.09 ± 0.01 | 14.8 ± 0.01 | 14.1 ± 0.5 | 17.6 ± 0.4 | 19.4 ± 0.4 | 20.0 ± 0.3 |
| FCC285 | 14.57 ± 0.03 | 13.15 ± 0.02 | 13.02 ± 0.03 | 12.77 ± 0.01 | 40.84 ± 1.63 | 46.78 ± 1.29 | 49.9 ± 1.54 | 51.1 ± 0.64 |
| FCC290 | 12.6 ± 0.095 | 11.4 ± 0.01 | 11.08 ± 0.01 | 10.74 ± 0.01 | 49.68 ± 0.53 | 49.65 ± 0.58 | 48.52 ± 0.16 | 48.41 ± 0.06 |
| FCC302 | 16.29 ± 0.09 | 15.58 ± 0.01 | 15.37 ± 0.04 | 15.06 ± 0.1 | 28.49 ± 1.7 | 21.92 ± 0.75 | 24.15 ± 0.78 | 28.84 ± 1.64 |
| FCC306 | 16.54 ± 0.02 | 15.29 ± 0.03 | 15.18 ± 0.01 | 15.0 ± 0.014 | 9.01 ± 0.16 | 10.52 ± 0.15 | 9.7 ± 0.06 | 9.85 ± 0.06 |
| FCC308 | 14.36 ± 0.02 | 12.87 ± 0.01 | 12.54 ± 0.01 | 12.17 ± 0.02 | 53.65 ± 1.41 | 44.91 ± 0.56 | 37.11 ± 0.82 | 46.46 ± 0.37 |
| FCC312 | 13.38 ± 0.05 | 11.4 ± 0.02 | 10.89 ± 0.09 | 10.45 ± 0.04 | 49.34 ± 2.13 | 76.0 ± 3.67 | 109.5 ± 9.33 | 117.8 ± 7.26 |
Notes. Column 1 – Fornax cluster members from Ferguson (1989); Columns 2 to 5 – Total magnitude in the u, g, r and i bands respectively, derived from the isophote fit. Values were corrected for the galactic extinction, using the absorption coefficient by Schlegel et al. (1998); Columns 6 to 9 – Effective radius in the u, g, r and i bands respectively, derived from the isophote fit.
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