The PAU Survey: Galaxy stellar population properties estimates with narrowband data

Open Access

Fig. 5.

Hexbin plots showing the ground truth from the PROSPECTOR-α stellar population simulations on the x-axis versus the MAP value from t PROSPECTOR, for stellar mass, M_*, current SFR, mean mass-weighted stellar ages, ⟨t_*⟩_m, stellar metallicity, Z_* and the optical depths of the two-component dust attenuation model, ${\hat{τ}}_{λ, 2}$ $\hat{\tau}_{\lambda, 2}$ and ${\hat{τ}}_{λ, 1}$ $\hat{\tau}_{\lambda,1}$ .

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