Table A.4.
Results of AGN and radio SED modeling using CIGALE.
| GMC | fAGN | accretion power | Ldisk | polar dust luminosity | RAGN | αAGN | αSF | qIR |
|---|---|---|---|---|---|---|---|---|
| [%] | [log10 erg s−1] | [log10 erg s−1] | [log10 erg s−1] | |||||
| 1 | 2.52 ± 1.37 | 32.70 ± 0.24 | 30.40 ± 0.24 | 31.97 ± 0.24 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.56 ± 0.11 | 2.20 ± 0.03 |
| 2 | 3.86 ± 2.56 | 33.01 ± 0.30 | 30.70 ± 0.31 | 32.28 ± 0.30 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.59 ± 0.12 | 2.20 ± 0.00 |
| 3 | 2.00 ± 0.01 | 34.01 ± 0.02 | 31.56 ± 0.10 | 33.28 ± 0.02 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.51 ± 0.04 | 2.21 ± 0.05 |
| 4 | 2.05 ± 0.46 | 34.48 ± 0.10 | 32.01 ± 0.10 | 33.75 ± 0.10 | 0.01 ± 0.01 | 0.70 ± 0.00 | 0.50 ± 0.00 | 2.20 ± 0.00 |
| 5 | 5.34 ± 1.48 | 34.87 ± 0.12 | 32.40 ± 0.12 | 34.13 ± 0.12 | 0.01 ± 0.01 | 0.70 ± 0.00 | 0.50 ± 0.00 | 2.20 ± 0.00 |
| 6 | 4.66 ± 2.68 | 34.31 ± 0.26 | 31.92 ± 0.24 | 33.57 ± 0.26 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.50 ± 0.00 | 2.20 ± 0.01 |
| 7 | 7.54 ± 2.85 | 33.79 ± 0.18 | 31.47 ± 0.25 | 33.06 ± 0.18 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.69 ± 0.11 | 2.64 ± 0.08 |
| 8 | 2.56 ± 1.54 | 33.18 ± 0.24 | 30.85 ± 0.25 | 32.45 ± 0.24 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.73 ± 0.12 | 2.22 ± 0.09 |
| 9 | 2.17 ± 0.93 | 32.95 ± 0.14 | 30.62 ± 0.22 | 32.22 ± 0.14 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.79 ± 0.11 | 2.20 ± 0.01 |
| 10 | 2.51 ± 1.42 | 32.97 ± 0.26 | 30.64 ± 0.25 | 32.23 ± 0.26 | 0.04 ± 0.04 | 0.70 ± 0.00 | 0.50 ± 0.00 | 2.58 ± 0.01 |
Notes. From left to right, the columns represents the GMC number, AGN fraction (fAGN), accretion power, disk luminosity (Ldisk), polar dust luminosity of AGN, radio loudness (RAGN), AGN power-law slope (αAGN), SF power-law slope (αSF), and radio-IR correlation parameter (qIR).
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