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Table 8.
Spearman correlation coefficients between the dust-corrected colours (mF365 − mF551)int and (mF551 − J)int and stellar population parameters (ρUV and ρVJ, respectively).
| BC03 |
BaSTI |
Padova00 |
||||
|---|---|---|---|---|---|---|
| ρUV | ρVJ | ρUV | ρVJ | ρUV | ρVJ | |
| AV | −0.90 | −0.80 | −0.95 | −0.77 | −0.91 | −0.67 |
| log10 Age | 0.61 | 0.23 | 0.30 | 0.17 | 0.46 | 0.07 |
| [M/H] | 0.68 | 0.84 | 0.24 | 0.75 | 0.46 | 0.80 |
| log10 sSFR | −0.98 | −0.55 | −0.98 | −0.75 | −0.96 | −0.67 |
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