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Table B.2.
The robustness of the recovery of the stellar population properties from the SED fitting test on mock SEDs that do not apply the mass-Z-age priors.
| Data cube | |||
|---|---|---|---|
| GALEX + LSST + Euclid | LSST + Euclid | Euclid-only | |
| Stellar mass density | |||
| μ | −0.03 | −0.03 | −0.02 |
| σ | 0.04 | 0.03 | 0.08 |
| ρ | 1.00 | 1.00 | 0.98 |
| Age | |||
| μ | −0.05 | −0.07 | −0.08 |
| σ | 0.04 | 0.03 | 0.04 |
| ρ | 0.97 | 0.96 | 0.97 |
| Metallicity | |||
| μ | −0.22 | −0.28 | −0.19 |
| σ | 0.10 | 0.10 | 0.05 |
| ρ | 0.13 | 0.30 | 0.81 |
| Dust optical depth | |||
| μ | 0.40 | 0.50 | 0.41 |
| σ | 0.22 | 0.23 | 0.17 |
| ρ | 0.17 | −0.04 | 0.03 |
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