Fig. 16.

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Inference on the latest HERA upper limits using the stacked LorEMU. Priors are shown in red, and the 95% contours of the posteriors in blue. The posteriors over the star formation parameters are identical to the corresponding priors, but in the case of fX, they show a significant departure from the prior. Models with low X-ray intensity (log10fX ≲ −0.6) are deemed less likely to match the observations by HERA.
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