Table A.2.
Input parameters used for the CIGALE SED fitting of the background galaxy in the tail of NGC 4330.
| Parameter | Value |
|---|---|
| Pop. synth. mod. | Bruzual & Charlot (2003) |
| Dust model | Draine et al. (2014) |
| IMF | Salpeter |
| Metallicity | 0.0001, 0.0004, 0.004, 0.008, 0.02, 0.05 |
| E(B − V)young | 0.1, 0.3, 0.5, 0.7, 1.0 |
| E(B − V)old | 0.44 |
| QPAH | 1.12, 2.5, 3.19, 4.58, 5.95 |
| α | 2.0 |
| γ | 0.02 |
Notes. Row 1: stellar population model. Row 2: dust emission model. Row 3: adopted initial mass function. Row 4: metallicity. Rows 5 and 6: V-band attenuation in the interstellar medium. Rows 7−9: dust model input parameters Mass fraction of PAH. The parameters for the final model that were used to trace the variation of the flux densities in the background galaxies are given in boldface.
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