Table 1.
Properties of the investigated galaxies and their GC systems.
| Name | d | logL | logM | Re | n | rbr | racc, N | racc, M | Re | rs, s | rs, f | rsh, s | rsh, f | RRB |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [L⊙] | [M⊙] | [kpc] | [kpc] | [rbr] | [rbr] | [rbr] | [rbr] | [rbr] | [rbr] | [rbr] | [rbr] | ||
| N 821 | 24 | 10.5 | 11.2 | 4.7 | 4.7 | 16 | 0.73 | 1.1 | 0.30 | 13 | 4.0 | 0.61 | 0.85 | 6.2 |
| N 1023 | 11.4 | 10.5 | 11.3 | 2.7 | 4.2 | 8.3 | 1.7 | 2.5 | 0.33 | 37 | 3.8 | 1.3 | 3.2 | – |
| N 1399 | 20 | 10.7 | 11.5 | 3.5 | 5.6 | 43 | 0.43 | 0.63 | 0.082 | 18 | 19 | 0.15 | 0.28 | – |
| N 1400 | 26 | 10.4 | 11.2 | 3.4 | 4.0 | 23 | 0.49 | 0.73 | 0.15 | 6.8 | 2.7 | 0.46 | 0.60 | 0.46 |
| N 1407 | 29 | 11 | 11.9 | 9.4 | 8.3 | 46 | 0.52 | 0.77 | 0.21 | 3.6 | 8.7 | – | 0.34 | 0.58 |
| N 2768 | 22 | 10.7 | 11.5 | 8.9 | 3.3 | 21 | 0.70 | 1.1 | 0.42 | 34 | 3.8 | 0.22 | 0.72 | 7.6 |
| N 3115 | 9.7 | 10.2 | 11.0 | 4.8 | 4.4 | 9.5 | 0.85 | 1.3 | 0.50 | 8.0 | 8.3 | 0.97 | 0.95 | – |
| N 3377 | 11.2 | 9.9 | 10.5 | 2.9 | 5.0 | 5.6 | 0.85 | 1.3 | 0.52 | 5.1 | 5.6 | 1.4 | 1.2 | 1.9 |
| N 4278 | 16 | 10.2 | 11.0 | 2.5 | 4.8 | 15 | 0.61 | 0.90 | 0.16 | 5.0 | 6.6 | 0.70 | 0.56 | 0.48 |
| N 4365 | 20 | 10.7 | 11.5 | 8.5 | 5.2 | 29 | 0.54 | 0.82 | 0.29 | 27 | 17 | 0.15 | 0.42 | 1.1 |
| N 4472 | 16.3 | 10.9 | 11.7 | 3.9 | 3.0 | 24 | 1.0 | 1.5 | 0.16 | 21 | 33 | – | 0.44 | – |
| N 4486 | 16 | 10.8 | 11.6 | 5.8 | 2.9 | 15 | 1.4 | 2.0 | 0.40 | 54 | 4.3 | 0.16 | 0.42 | – |
| N 4494 | 17.1 | 10.4 | 11.1 | 3.7 | 3.4 | 10 | 1.0 | 1.5 | 0.36 | 11 | 3.9 | 1.0 | 1.5 | – |
| N 4526 | 17 | 10.4 | 11.2 | 2.7 | 3.6 | 12 | 1.0 | 1.5 | 0.22 | 13 | 6.5 | 0.92 | 0.99 | – |
| N 4649 | 17 | 10.8 | 11.6 | 5.1 | 3.6 | 30 | 0.69 | 1.0 | 0.17 | 25 | 11 | 0.074 | 0.53 | – |
| N 5128 | 4.2 | 10.5 | 11.2 | 6.2 | 4.0 | 12 | 0.93 | 1.4 | 0.54 | 18 | 22 | 0.77 | 0.65 | – |
| N 5846 | 25 | 10.7 | 11.6 | 8.1 | 3.9 | 37 | 0.44 | 0.68 | 0.22 | 21 | 8.5 | 0.099 | 0.30 | 0.77 |
| R17x | 19 | 10.2 | 11.0 | 1.5 | 2.6 | 2.0 | 5.2 | 7.4 | 0.75 | 38 | 16 | 6.0 | 10 | – |
| R17y | 19 | 10.2 | 11.0 | 1.7 | 2.0 | 3.0 | 3.6 | 5.1 | 0.57 | 26 | 13 | 4.1 | 5.7 | – |
| R17z | 19 | 10.2 | 11.0 | 2.0 | 2.0 | 3.4 | 3.1 | 4.4 | 0.58 | 22 | 9.2 | 3.5 | 4.3 | – |
Notes. d – Galaxy distance. L – Galaxy B-band luminosity. M – Galaxy stellar mass. Re – Sérsic effective radius. n – Sérsic index. rbr – Break radius of the number density profile of the GC system. racc, N – Radius where the Newtonian acceleration equals a0. racc, M – Radius where the MOND acceleration equals a0. rs, s – Scale radius of a NFW halo following the scaling relations calculated from the stellar mass. rs, f – Scale radius of a NFW halo obtained by Bílek et al. (2019) from fitting the GC kinematics. rsh, s – Radius at which the acceleration originating from the stars and the dark halo are equal. The halo parameters were estimated from the scaling relations. A dash means that the acceleration exerted by dark matter is stronger than the acceleration exerted by the stars at all radii. rsh, f – The same, but the halo parameters were estimated by fitting the GC kinematics. RRB – Radius where surface densities of the red and blue GCs are equal. A dash means missing data.
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