A halo model approach to describe clustering and emission of the two main star-forming galaxy populations for cosmic infrared background studies

Open Access

Fig. 4.

Posterior probability distributions of the clustering parameters for the two scenarios where the correlations for the shot noise are fixed to unity (in purple) and where they are free parameters in the fit (in green). The posterior distributions for the two cases are in agreement, exploring the same regions of the parameter space. We fix $α_{ET} = 1$ $\alpha_{{\rm{ET}}} = 1$ .

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