Table E.1
Significance level of the Kolmogorov-Smirnov statistic between two subsamples of barred and non-barred galaxies studied as a function of the stellar-to-halo mass ratio.
| K-S p-value | 8.5 < log10(M∗/M⊙) < 9 | 9 < log10(M∗/M⊙) < 9.5 | 9.5 < log10(M∗/M⊙) < 10 | 10 < log10(M∗/M⊙) < 10.5 | 10.5 < log10(M∗/M⊙) < 11 |
|
|
|||||
| Visual | 0.63 | 0.17 | 0.01 | 0.25 | 0.55 |
| Ellipse fitting | 0.34 | 0.02 | 0.32 | 0.25 | 0.11 |
∃ & Qb |
0.81 | 0.03 | 0.15 | 0.63 | 0.14 |
|
|
|||||
| rbar> 0.9hR | |||||
| Visual | 0.36 | 0.28 | 0.04 | 0.16 | 0.29 |
| Ellipse fitting | 0.34 | 0.20 | 0.47 | 0.09 | 0.09 |
| ∃ & Qb |
0.68 | 1.00 | 0.38 | 0.19 | 0.18 |
|
|
|||||
| rbar ≤ 0.9hR | |||||
| Visual | 0.52 | 0.26 | 0.01 | 0.69 | 0.46 |
| Ellipse fitting | 0.43 | 0.03 | 0.54 | 0.68 | 0.14 |
| ∃ & Qb |
0.00 | 0.00 | 0.08 | 0.74 | 0.21 |
|
|
|||||
|
|||||
| Visual | 0.85 | 0.11 | 0.07 | 0.11 | 0.27 |
| Ellipse fitting | 0.93 | 0.02 | 0.42 | 0.10 | 0.36 |
| ∃ & Qb |
0.99 | 0.04 | 0.44 | 0.29 | 0.44 |
|
|
|||||
|
|||||
| Visual | 0.09 | 0.47 | 0.00 | 0.67 | 0.22 |
| Ellipse fitting | 0.21 | 0.09 | 0.31 | 0.72 | 0.01 |
| ∃ & Qb |
0.45 | 0.35 | 0.01 | 0.80 | 0.03 |
Notes. The subsamples were drawn from the stellar mass bins shown in the lower panel of Fig. 19 (the M∗ thresholds are displayed in the first row). K-S tests are also performed for galaxies with relative bar sizes lower or greater than the median rbar/hR and also for the different bar families (SAB and 
B on one side, and SB and SA
on the other), all of them compared to the family of non-barred galaxies. In general, the distribution of Mh/M∗ is not significantly different for barred and non barred galaxies (regardless of size and strength), given a certain stellar mass range (indicated by p-values ≥0.01).
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