Table 4.
Comparison of the best MOND and ΛCDM fits.
| Name | ΛCDM | MOND | ΔAICc | ΛCDM | MOND | ΔLBF | ||||
|---|---|---|---|---|---|---|---|---|---|---|
| β | AICc | β | AICc | β | LBF | β | LBF | |||
| N 821 | lit | –51.2 | lit | –56.4 | 5.2 | lit | 10.8 | lit | 11.4 | –0.55 |
| N 1023 | lit | –106 | lit | –109 | 4.0 | lit | 22.8 | lit | 23.0 | –0.17 |
| N 1399 | neg | 431 | neg | 556 | –120 | neg | –95.0 | neg | –195 | 100 |
| N 1400 | neg | –76.0 | neg | –80.1 | 4.2 | neg | 16.5 | neg | 16.8 | –0.35 |
| N 1407 | neg | 12.8 | neg | 30.0 | –17 | neg | –3.92 | neg | –7.54 | 3.6 |
| N 2768 | lit | –84.4 | lit | –91.5 | 7.0 | lit | 18.1 | lit | 19.1 | –1.0 |
| N 3115 | lit | –106 | neg | –110 | 3.6 | lit | 22.5 | neg | 22.6 | –0.098 |
| N 3377 | lit | –215 | iso | –219 | 3.5 | lit | 46.2 | iso | 46.3 | –0.12 |
| N 4278 | iso | –147 | neg | –145 | –1.7 | iso | 31.1 | neg | 30.4 | 0.73 |
| N 4365 | lit | 14.3 | neg | 35.7 | –21 | lit | –4.02 | neg | –8.85 | 4.8 |
| N 4472 | neg | 170 | neg | 199 | –29 | neg | –38.2 | neg | –45.7 | 7.5 |
| N 4486 | neg | 535 | neg | 593 | –58 | neg | –121 | neg | –142 | 21 |
| N 4494 | iso | –178 | iso | –180 | 1.5 | iso | 38.5 | lit | 38.0 | 0.45 |
| N 4526 | neg | –52.8 | neg | –57.3 | 4.5 | neg | 11.3 | neg | 11.7 | –0.37 |
| N 4649 | iso | 41.2 | neg | 43.6 | –2.4 | neg | –9.98 | neg | –10.6 | 0.66 |
| N 5128 | neg | –419 | neg | –378 | –41 | neg | 89.4 | neg | 80.7 | 8.7 |
| N 5846 | neg | 16.5 | neg | 31.5 | –15 | neg | –4.30 | neg | –7.63 | 3.3 |
| R17x | neg | –267 | lit | –268 | 1.6 | neg | 57.6 | lit | 57.3 | 0.28 |
| R17y | lit | –257 | lit | –260 | 2.9 | lit | 55.4 | lit | 55.4 | 0.037 |
| R17z | lit | –277 | lit | –280 | 3.5 | lit | 59.9 | lit | 59.9 | –0.0072 |
Notes. Lower AICc value and higher LBF value indicate the better fit. In the columns ΔAICc and ΔLBF, the cases where the ΛCDM models performed better than the MOND models with respect to the given criterion are highlighted by boldface. We note that the three last galaxies are not real; they come from a simulation (see Sect. 2). The number of galaxies for which the MOND models are preferred is comparable to that of the galaxies where the ΛCDM models are preferred. If the values of the preference are compared, the ΛCDM models come out more successful.
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