A self-consistent population synthesis using ray-tracing and simulation-based inference simultaneously reproduces the cosmic X-ray background and AGN absorption statistics, yielding an intrinsic Compton-thick fraction of 21 plus or minus 7 percent.
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Self-consistent population synthesis of AGN from observational constraints in the X-rays
A self-consistent population synthesis using ray-tracing and simulation-based inference simultaneously reproduces the cosmic X-ray background and AGN absorption statistics, yielding an intrinsic Compton-thick fraction of 21 plus or minus 7 percent.