Table 3.
Total magnitudes and effective radii for the early-type galaxies inside the virial radius (Rvir ∼ 0.7 Mpc) of the Fornax cluster, brighter than mB < 15 mag, in the ugri bands.
| 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) |
| FCC 090 | 15.18 ± 0.04 | 14.16 ± 0.02 | 13.62 ± 0.03 | 13.38 ± 0.02 | 10.34 ± 0.10 | 10.31 ± 0.06 | 12.11 ± 0.10 | 11.31 ± 0.07 |
| FCC 143 | 14.88 ± 0.06 | 13.36 ± 0.02 | 12.66 ± 0.03 | 12.39 ± 0.07 | 13.51 ± 0.09 | 11.86 ± 0.01 | 11.00 ± 0.05 | 10.46 ± 0.09 |
| FCC 147 | 12.67 ± 0.03 | 11.14 ± 0.01 | 10.50 ± 0.01 | 10.15 ± 0.02 | 38.34 ± 0.12 | 28.53 ± 0.01 | 24.8 ± 0.2 | 24.1 ± 0.2 |
| FCC 148 | 13.77 ± 0.02 | 12.33 ± 0.01 | 11.70 ± 0.01 | 11.47 ± 0.02 | 30.4 ± 0.2 | 27.2 ± 0.2 | 28.3 ± 0.2 | 25.04 ± 0.14 |
| FCC 153 | 13.88 ± 0.02 | 11.94 ± 0.02 | 11.70 ± 0.03 | 11.17 ± 0.01 | 24.5 ± 0.3 | 26.3 ± 0.3 | 19.8 ± 0.7 | 27.4 ± 0.5 |
| FCC 161 | 12.85 ± 0.03 | 11.18 ± 0.01 | 10.47 ± 0.01 | 10.14 ± 0.03 | 28.2 ± 0.2 | 28.6 ± 0.2 | 28.6 ± 0.2 | 26.96 ± 0.03 |
| FCC 167 | 11.70 ± 0.02 | 9.86 ± 0.01 | 9.27 ± 0.02 | 8.83 ± 0.01 | 57.9 ± 0.3 | 72.7 ± 0.5 | 56.4 ± 0.5 | 60.0 ± 0.4 |
| FCC 170 | 13.30 ± 0.01 | 11.64 ± 0.01 | 10.99 ± 0.01 | 10.57 ± 0.01 | 20.9 ± 0.5 | 17.97 ± 0.15 | 15.89 ± 0.13 | 16.34 ± 0.12 |
| FCC 177 | 13.88 ± 0.04 | 12.52 ± 0.01 | 11.8 ± 0.01 | 11.44 ± 0.02 | 31 ± 1 | 33.9 ± 0.3 | 35.9 ± 0.2 | 35.6 ± 0.2 |
| FCC 182 | 15.66 ± 0.04 | 14.24 ± 0.01 | 13.58 ± 0.01 | 13.21 ± 0.01 | 12.66 ± 0.05 | 10.27 ± 0.05 | 9.90 ± 0.05 | 9.78 ± 0.06 |
| FCC 184 | 12.64 ± 0.01 | 10.76 ± 0.01 | 10.00 ± 0.04 | 9.62 ± 0.03 | 32.26 ± 0.03 | 36.8 ± 0.01 | 34.45 ± 0.01 | 31.17 ± 0.11 |
| FCC 190 | 14.20 ± 0.06 | 12.92 ± 0.01 | 12.26 ± 0.01 | 11.88 ± 0.01 | 26.32 ± 0.13 | 18.98 ± 0.08 | 18.34 ± 0.08 | 18.2 ± 0.08 |
| FCC 193 | 13.09 ± 0.06 | 11.42 ± 0.01 | 10.69 ± 0.02 | 10.25 ± 0.02 | 28.2 ± 0.3 | 27.6 ± 0.3 | 28.2 ± 0.3 | 32.8 ± 0.4 |
| FCC 213 | 10.55 ± 0.12 | 8.57 ± 0.09 | 7.89 ± 0.09 | 7.59 ± 0.03 | 232 ± 2 | 346 ± 3 | 308 ± 2 | 248 ± 2 |
| FCC 219 | 11.33 ± 0.04 | 9.28 ± 0.08 | 8.57 ± 0.04 | 8.32 ± 0.01 | 97.47 ± 0.06 | 201.5 ± 0.1 | 161 ± 0.2 | 116.6 ± 0.9 |
| FCC 276 | 12.52 ± 0.05 | 10.45 ± 0.06 | 10.15 ± 0.02 | 9.81 ± 0.04 | 56.1 ± 0.5 | 56.1 ± 0.5 | 44.67 ± 0.07 | 42.4 ± 0.3 |
| FCC 277 | 14.64 ± 0.02 | 12.74 ± 0.01 | 12.34 ± 0.02 | 11.97 ± 0.04 | 14.45 ± 0.10 | 12.61 ± 0.05 | 12.78 ± 0.04 | 12.61 ± 0.03 |
| FCC 301 | 15.0 ± 0.1 | 12.99 ± 0.05 | 12.65 ± 0.01 | 12.29 ± 0.03 | 14.9 ± 0.4 | 13.7 ± 0.4 | 11.7 ± 0.3 | 11.9 ± 0.3 |
| FCC 310 | 13.0 ± 0.01 | 12.19 ± 0.05 | 11.81 ± 0.04 | 11.41 ± 0.01 | 63 ± 1 | 36.3 ± 0.14 | 35.57 ± 0.02 | 36.41 ± 0.06 |
Notes. Column 1: Fornax cluster members from Ferguson (1989). Columns 2–5: total magnitudes in the u, g, r, and i band respectively, derived from the isophote fit. Values were corrected for the Galactic extinction by using the absorption coefficient by Schlegel et al. (1998). Columns 6–9: effective radius in the u, g, r, and i band respectively, derived from the isophote fit.
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