Table 3.
Comparison of the estimation of the physical parameters.
| Parameter | Mean (1σ) [min, max] | 58 fluxes added (1σ) |
|---|---|---|
| Mass of the bursting population (107 M⊙) | 17.04 (±4.50) [0.01, 2.76] | 12.05 (±2.42) |
| V-band attenuation | 0.73 (±0.08) [0.23, 2.07] | 0.68 (±0.10) |
| Power law slope of dust attenuation in the ISM | −0.62 (∓0.25) [−1.07, −0.22] | −0.70 (∓0.22) |
| PAH fraction | 3.16 (±0.46) [0.49, 5.35] | 2.86 (±0.58) |
| Star formation rate (M⊙ yr−1) | 8.50 (±1.01) [0.03, 0.70] | 8.21 (±1.53) |
| Stellar mass (109 M⊙) | 45.8 (±13.0) [0.2, 3.1] | 40.5 (±9.5) |
Notes. The values of the SFR, stellar mass, and mass of the bursting population of the 58 regions in the second column are added together to allow for a comparison with integrated values. Thus, the minimum and maximum of these parameters correspond to the lowest and highest values out of the 58 regions.
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