Table B.2
Bayesian information criterion weight values for all clouds and for all models. The most likely model is denoted by its weight being bold. If the second most likely model has a weight within a factor of 10 of the most likely model (i.e. may be an alternative model) it is shown with an italic, bold weight. We note that for Draco, no PLT could be fit, the most likely model is the ELL one with a weight of 9.826514e−01. Other models (EL, L, LL, LP etc.) have higher weights.
| Model | ELP | ELLP | EL2P | ELL2P | LP | LLP | L2P | LL2P |
|---|---|---|---|---|---|---|---|---|
| High-mass SF regions | ||||||||
| Cygnus North | 5.946e−90 | 4.692e−10 | 4.741e−43 | 1.000e+00 | 0.000e+00 | 2.039e−208 | 0.000e+00 | 1.393e−161 |
| Cygnus South | 1.202e−67 | 8.924e−03 | 1.233e−65 | 9.911e−01 | 0.000e+00 | 3.067e−290 | 0.000e+00 | 1.926e−288 |
| M16 | 1.708e−122 | 1.000e+00 | 1.526e−90 | 3.916e−29 | 0.000e+00 | 1.544e−50 | 0.000e+00 | 6.596e−76 |
| M17 | 0.000e+00 | 1.409e−36 | 0.000e+00 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 |
| NGC6334 | 0.000e+00 | 3.432e−67 | 0.000e+00 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 |
| NGC6357 | 0.000e+00 | 5.933e−06 | 0.000e+00 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 |
| NGC7538 | 9.348e−120 | 2.554e−30 | 2.834e−20 | 1.000e+00 | 0.000e+00 | 1.212e−146 | 0.000e+00 | 3.111e−145 |
| Rosette | 2.911e−99 | 8.076e−07 | 6.816e−29 | 9.999e−01 | 0.000e+00 | 1.177e−155 | 0.000e+00 | 1.665e−157 |
| Vela C | 2.477e−202 | 1.905e−54 | 9.547e−103 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 1.846e−96 |
| Intermediate−mass SF regions | ||||||||
| Aquila | 5.982e−102 | 3.158e−29 | 2.212e−73 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 |
| MonR2 | 3.485e−158 | 9.099e−96 | 6.163e−13 | 1.000e+00 | 0.000e+00 | 4.813e−45 | 0.000e+00 | 6.355e−21 |
| MonOB1 | 0.000e+00 | 3.207e−64 | 0.000e+00 | 1.000e+00 | 0.000e+00 | 4.076e−207 | 0.000e+00 | 1.425e−106 |
| NGC2264 | 1.302e−44 | 3.127e−31 | 2.960e−31 | 1.000e+00 | 0.000e+00 | 3.198e−146 | 0.000e+00 | 1.857e−224 |
| Orion B | 6.236e−151 | 2.609e−137 | 2.152e−16 | 1.000e+00 | 5.771e−150 | 1.661e−146 | 1.672e−15 | 1.810e−11 |
| Serpens | 6.480e−220 | 1.063e−12 | 8.833e−100 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 | 0.000e+00 |
| Low-mass SF regions | ||||||||
| ChamI | 0.000e+00 | 2.148e−52 | 1.000e+00 | 1.007e−18 | 0.000e+00 | 2.905e−283 | 0.000e+00 | 1.694e−258 |
| ChamII | 3.479e−167 | 7.628e−22 | 9.050e−150 | 1.000e+00 | 0.000e+00 | 4.814e−47 | 8.000e−81 | 1.051e−27 |
| IC5146 | 0.000e+00 | 0.000e+00 | 5.121e−127 | 1.000e+00 | 0.000e+00 | 0.000e+00 | 8.918e−154 | 2.501e−22 |
| Lupus I | 3.243e−34 | 5.491e−25 | 1.524e−03 | 9.985e−01 | 0.000e+00 | 1.176e−100 | 0.000e+00 | 1.439e−126 |
| Lupus III | 9.158e−85 | 1.174e−04 | 3.702e−17 | 9.999e−01 | 1.705e−100 | 3.623e−30 | 1.131e−34 | 2.992e−14 |
| Lupus IV | 2.238e−68 | 2.267e−13 | 1.567e−23 | 1.000e+00 | 2.905e−103 | 1.930e−61 | 6.169e−83 | 6.104e−17 |
| Perseus | 3.530e−133 | 2.099e−21 | 1.725e−02 | 1.444e−03 | 0.000e+00 | 7.782e−26 | 9.792e−01 | 2.134e−03 |
| Pipe | 1.308e−49 | 4.531e−15 | 3.919e−13 | 3.578e−01 | 7.876e−49 | 1.242e−21 | 1.315e−16 | 6.422e−01 |
| Taurus | 0.000e+00 | 0.000e+00 | 3.708e−15 | 1.116e−01 | 0.000e+00 | 0.000e+00 | 1.042e−56 | 8.884e−01 |
| Quiescent regions | ||||||||
| ChamIII | 2.261e−130 | 2.989e−04 | 1.223e−107 | 9.997e−01 | 7.567e−166 | 1.427e−37 | 1.229e−105 | 5.326e−34 |
| Musca | 0.000e+00 | 7.418e−02 | 1.469e−10 | 2.078e−01 | 0.000e+00 | 4.063e−38 | 2.941e−29 | 7.180e−01 |
| Polaris | 1.931e−25 | 5.520e−02 | 1.197e−22 | 9.448e−01 | 1.843e−36 | 2.702e−10 | 1.504e−31 | 1.450e−09 |
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