Table 3.
Best-fit results for the g band.
| Name | mag_g | Reff [arcsec] | n | b/a | PA | L [109 L⊙] |
|---|---|---|---|---|---|---|
| NGC5098a | 15.3937 ± 0.0086 | 3.64 ± 0.02 | 2.116 ± 0.007 | 1.00 | 40.18 | 22.3 |
| NGC5098a | 13.7793 ± 0.0038 | 52.19 ± 0.15 | 2.677 ± 0.021 | 0.92 | 28.33 | 98.4 |
| NGC5098b | 14.5652 ± 0.0008 | 6.67 ± 0.01 | 3.248 ± 0.005 | 0.89 | 34.71 | 47.7 |
| LEDA2024371 | 15.9482 ± 0.0011 | 3.16 ± 0.01 | 3.758 ± 0.012 | 0.81 | 88.22 | 13.4 |
| LEDA2024547 | 17.2384 ± 0.0020 | 2.61 ± 0.01 | 2.553 ± 0.014 | 0.82 | −83.27 | 4.07 |
| LEDA2023331 | 16.9627 ± 0.0032 | 6.37 ± 0.01 | 0.244 ± 0.002 | 0.25 | 42.79 | 5.25 |
| LEDA2023331 | 15.5242 ± 0.0010 | 4.92 ± 0.01 | 3.385 ± 0.007 | 0.82 | 27.55 | 19.7 |
| LEDA2023332 | 15.0016 ± 0.0007 | 6.62 ± 0.01 | 4.502 ± 0.008 | 0.54 | −49.60 | 31.9 |
| NGC5096s | 13.7989 ± 0.0025 | 37.95 ± 0.25 | 9.201 ± 0.023 | 0.81 | 88.57 | 96.7 |
| NGC5096n | 15.8877 ± 0.0016 | 2.14 ± 0.01 | 4.563 ± 0.024 | 0.56 | 12.42 | 14.1 |
| NGC5096w | 16.9535 ± 0.0076 | 0.98 ± 0.01 | 2.553 ± 0.047 | 0.64 | −62.69 | 5.29 |
| NGC5096w | 17.2145 ± 0.0091 | 3.89 ± 0.02 | 0.797 ± 0.008 | 0.90 | −49.68 | 4.16 |
| LEDA2023056 | 15.6807 ± 0.0018 | 6.16 ± 0.03 | 5.212 ± 0.028 | 0.45 | −69.69 | 17.1 |
| LEDA2023056 | 16.6541 ± 0.0038 | 8.50 ± 0.01 | 0.479 ± 0.003 | 0.24 | −71.84 | 6.97 |
| LEDA2023215 | 16.9351 ± 0.0017 | 4.52 ± 0.01 | 0.896 ± 0.004 | 0.36 | −46.28 | 5.38 |
| LEDA2024686 | 15.9819 ± 0.0011 | 6.18 ± 0.01 | 0.902 ± 0.002 | 0.28 | −42.70 | 3.23 |
Notes. Two consecutive lines mean that a double-Sérsic model was used. The galaxies follow the same order as in Table 2. The total magnitude for each model is mag_g, Reff is the effective radius, n is the Sérsic index, b/a is the axial ratio, and PA is the position angle measured from north to east. Error bars are 1σ confidence level. For LEDA2024686 we assume a luminosity distance of 85 Mpc.
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