Reconciling PTA and JWST, and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations

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Fig. 2.

Stochastic GW background predicted by our model (green) and the free spectrum measured by EPTA (blue). The 90% confidence intervals centred at the median for the amplitude of the GW background in the first and last bins, i.e., at frequencies 1/(10 yr) and 1/(1 yr), are $4 . 8_{- 2.7}^{+ 5.1} \times 10^{- 15}$ $4.8^{+5.1}_{-2.7}\times 10^{-15}$ and $1 . 0_{- 0.6}^{+ 1.1} \times 10^{- 15}$ $1.0^{+1.1}_{-0.6}\times 10^{-15}$ , respectively.

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