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

Open Access

Fig. A.1.

Posterior distribution of an example galaxy with non-converged properties from PROSPECTOR. The properties shown are the metallicity, the diffuse dust optical depths ${\hat{τ}}_{λ}$ $\hat{\tau}_{\lambda}$ , the ratio between diffuse dust and birth cloud optical depths, the dust slope modifier, n, the stellar mass, and the ratios of SFRs between adjacent age bins, which define the non-parametric SFH.

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