Table A.2
Luminosity weighted-averaged and slopes of the U, n, and cut1 (ionized gas), and cut2 (neutral gas) parameters of the power law models.
| Galaxy | log <n>(1) | log <U>(2) |  |
 |
<cut1>(4) | <cut2>(5) |  |
 |
Pclumpy |
|---|---|---|---|---|---|---|---|---|---|
| Haro2 |  |
 |
 |
 |
 |
 |
 |
 |
0.30 |
| Haro3 |  |
 |
 |
 |
 |
 |
 |
 |
0.24 |
| Haro11 |  |
 |
 |
 |
 |
 |
 |
 |
0.005 |
| He2-10 |  |
 |
 |
 |
 |
 |
 |
 |
0.71 |
| IIZw40 |  |
 |
 |
 |
 |
 |
 |
 |
0.40 |
| IZw18 |  |
 |
 |
 |
 |
 |
 |
 |
0.47 |
| Mrk209 |  |
 |
 |
 |
 |
 |
 |
 |
0.75 |
| Mrk930 |  |
 |
 |
 |
 |
 |
 |
 |
0.03 |
| Mrk1089 |  |
 |
 |
 |
 |
 |
 |
 |
0.25 |
| NGC1140 |  |
 |
 |
 |
 |
 |
 |
 |
0.01 |
| NGC1569 |  |
 |
 |
 |
 |
 |
 |
 |
0.06 |
| NGC1705 |  |
 |
 |
 |
 |
 |
 |
 |
0.23 |
| NGC5253 |  |
 |
 |
 |
 |
 |
 |
 |
0.02 |
| NGC625 |  |
 |
 |
 |
 |
 |
 |
 |
0.19 |
| SBS0335 |  |
 |
 |
 |
 |
 |
 |
 |
0.05 |
| UM448 |  |
 |
 |
 |
 |
 |
 |
 |
0.003 |
| UM461 |  |
 |
 |
 |
 |
 |
 |
 |
0.58 |
| VIIZw403 |  |
 |
 |
 |
 |
 |
 |
 |
0.49 |
The reported errorbars for weighted-averages correspond to the upper bound and lower boundaries of the power law, and to the High Density Probability Interval at 94% for the slopes. Galaxies flagged in bold with maximum cuts larger than 2 and negative 
slopes correspond to clumpy galaxies, as defined by Equation 11.
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