Table A.3.
Dust and SFH related results obtained from SED modeling with CIGALE, including AGN component.
| GMC | Mdust | Umin | γ | qPAH | ageburst | fburst | τburst | τmain |
|---|---|---|---|---|---|---|---|---|
| [log10 (M⊙)] | [Myr] | [Myr] | [Myr] | |||||
| 1 | 4.47 ± 0.09 | 4.39 ± 1.51 | 0.025 ± 0.033 | 2.236 ± 0.590 | 7.87 ± 99.45 | 0.03 ± 0.02 | 142.23 ± 85.13 | 1170.23 ± 645.23 |
| 2 | 4.49 ± 0.09 | 3.06 ± 1.84 | 0.057 ± 0.067 | 4.821 ± 1.218 | 8.10 ± 32.48 | 0.02 ± 0.01 | 210.26 ± 75.10 | 290.93 ± 141.61 |
| 3 | 5.89 ± 0.07 | 3.25 ± 0.72 | 0.011 ± 0.010 | 1.118 ± 0.036 | 7.74 ± 98.75 | 0.03 ± 0.02 | 126.62 ± 81.91 | 864.58 ± 527.05 |
| 4 | 6.19 ± 0.04 | 0.68 ± 0.16 | 0.089 ± 0.038 | 0.470 ± 0.001 | 8.16 ± 8.01 | 0.01 ± 0.00 | 246.94 ± 60.90 | 203.13 ± 30.50 |
| 5 | 6.23 ± 0.09 | 0.90 ± 0.39 | 0.078 ± 0.025 | 0.471 ± 0.026 | 7.92 ± 0.01 | 0.01 ± 0.02 | 180.44 ± 84.63 | 213.33 ± 61.83 |
| 6 | 6.08 ± 0.06 | 0.58 ± 0.34 | 0.189 ± 0.033 | 1.036 ± 0.312 | 7.93 ± 101.79 | 0.03 ± 0.02 | 170.89 ± 86.57 | 1520.01 ± 683.09 |
| 7 | 5.13 ± 0.11 | 9.03 ± 1.47 | 0.192 ± 0.029 | 3.116 ± 0.871 | 7.68 ± 93.06 | 0.03 ± 0.02 | 134.24 ± 83.65 | 844.18 ± 544.03 |
| 8 | 4.79 ± 0.21 | 2.65 ± 1.02 | 0.160 ± 0.053 | 3.384 ± 1.132 | 7.75 ± 88.29 | 0.02 ± 0.01 | 176.04 ± 86.66 | 258.82 ± 125.10 |
| 9 | 4.73 ± 0.23 | 5.37 ± 1.72 | 0.012 ± 0.014 | 3.105 ± 0.838 | 7.71 ± 93.91 | 0.03 ± 0.02 | 137.08 ± 83.70 | 592.04 ± 305.75 |
| 10 | 4.83 ± 0.19 | 1.87 ± 0.71 | 0.051 ± 0.042 | 3.412 ± 0.918 | 7.82 ± 103.06 | 0.02 ± 0.02 | 170.82 ± 86.23 | 589.30 ± 352.26 |
Notes. From left to right columns are: the GMC number, the dust mass (Mdust), the minimum radiation field (Umin), the fraction illuminated from Umin to the maximum radiation field (γ), the mass fraction of PAH (qPAH), the age of the late burst (ageburst), the mass fraction of late burst population (fburst), the e-folding time of the late starburst population model (τburst) and that of the main stellar population model (τmain).
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