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Fig. 6


Luminosity function, from combined XMM-LSS, CDFS, and COSMOS data, with binned estimates (black data points with 1σ error bars) and Bayesian highest posterior densities (HPD) under the LDDE (blue area) and LADE (red area) models. For both models, the darker areas show the 68.3% HPD intervals, while the lighter areas show the 99.7% HPD intervals.

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