Table E.1
Model parameters of the 9 BCGs that are considered here.
| Low surface-brightness component | Starburst component | ||||||||||||||
| Galaxy | D | Band | n | r e | h | μ | n | r e | h | Δμ | r X | Ref. | Figures | ||
|
|
|||||||||||||||
| ESO 400-G043 | 77 | B | 17.1 | 1.13 mas | – | −38.85 | – | – | – | – | – | 1a | 6 | ||
| 77 | B | 1 | 11 | 6.7 | 23.1 | – | – | – | – | – | 1a | 6 | |||
| 79.2 | V | 1 | 7.21 | 4.31 | 20.64 | – | – | – | – | – | 2b | 6 | |||
| 79.2 | V | 1 | 15.7 | 9.39 | 23.60 | – | – | – | – | – | 2c | 6 | |||
| 79.2 | 1 | 4.3 | 2.6 | – | 1 | 1.5 | 0.90 | 4.75 | 5.0 | 6 | |||||
| Mrk 5 | 13.3 | B | 1 | 8.02 | 4.81 | 21.09 | – | – | – | – | – | 3d | 8 | ||
| UGCA 130 | 13.3 | B | 2.83 | 3.35 | – | 20.23 | – | – | – | – | – | 4 | 8 | ||
| 13.96 | B | 0.99 | 9.6 | – | 21.18 | – | – | – | – | – | 5 | 8 | |||
| 13.3 | 1 | 8.0 | 4.8 | – | 1 | 2.0 | 1.2 | 0.7 | – | 8 | |||||
| ESO 350-IG038 | 80 | B | 19.8 | 0.080 mas | – | −53.95 | – | – | – | – | – | 1e | E.1 | ||
| Haro 11 | 80 | B | 1 | 14 | 8.3 | 23.5 | – | – | – | – | – | 1e | E.1 | ||
| 82 | 1 | 5.0 | 3.0 | – | 1 | 0.7 | 0.42 | 8.50 | 2.5 | E.1 | |||||
| 82 | 11.0 | 8.25 mas | – | −41.20 | – | – | – | – | – | E.4 | |||||
| Mrk 297 f | 63 | B | 1 | 16.3 | 9.72 | 22.43 | – | – | – | – | – | 6 | E.2 | ||
| NGC 6052/54 | 64.3 | B | 1 | 13.3 | 7.96 | 22.30 | – | – | – | – | – | 3g | E.2 | ||
| UGC 10182 | 65.10 | B | 0.84 | 9.25 | – | 21.35 | – | – | – | – | – | 5 | E.2 | ||
| 64.3 | , 3.5, 18.48, 16.6, 16, 22h | 1 | 2.0 | 1.2 | – | – | E.2 | ||||||||
| UM 465 | 20.7 | B | 1 | 10.8 | 6.48 | 19.97 | – | – | – | – | – | 7b | E.3 | ||
| UGC 6877 | 20.7 | B | 1 | 15.7 | 9.37 | 21.82 | – | – | – | – | – | 7c | E.3 | ||
| Mrk 1308 | 20.7 | 1 | 9.53 | 5.70 | – | 1 | 2.5 | 1.5 | 2.4 | – | E.3 | ||||
| VCC 0001 | 32 | r | 1 | 2.6 | 1.5 | 20.3 | – | – | – | – | – | 8 | E.5 | ||
| 32 | 1 | 4.9 | 2.9 | – | – | – | – | – | – | E.5 | |||||
Notes. Only those values where a value is provided are shown. The distances are in this work only used to scale the upper x-axis in the surface-brightness profile plots. Details of the original observations are given in Table A.1. Column 1, galaxy name, some alternative names are provided indented on subsequent lines; Col. 2, distance (Mpc); Col. 3, bandpass used in the observations; Cols. 4–7, Sérsic parameters of the low surface-brightness component in the form of the index, the half-light radius (arcsec), the corresponding scale length when n ≡ 1 (arcsec), and the intensity at r = 0 (n = 1) or re (mag arcsec-2, n ≠ 1); Cols. 8–11, Sérsic parameters of the starburst component in the form of the index, the half-light radius (arcsec), the corresponding scale length when n ≡ 1 (arcsec), and the magnitude difference Δμ = μ − μe (mag arcsec-2); Col. 12, inner truncation radius (arcsec); Col. 13, references, rows without a number refer to this study; and Col. 14, results are shown in this figure.
The scale length and the central surface brightness are based on measurements in the radial range where 24 ≤ μ ≤ 26 mag arcsec-2.
The scale length and the central surface brightness are based on measurements in the radial range where 26 ≤ μ ≤ 28 mag arcsec-2.
Besides the low surface-brightness component, the parameters of the two inner components are given in Sect. E.2.
The six values specify the five face-on galaxy parameters hi (arcsec), ho (arcsec), μ0,i (mag arcsec-2), μ0,o (mag arcsec-2), and rbr (arcsec), as well as μe of the bulge (mag arcsec-2).
Reference. (1) BÖ02; (2) M13a; (3) C01; (4) C05; (5) Amorín et al. (2009); (6) P96; (7) M13b; (8) Meyer et al. (2014).
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