Measuring photo-ionization rate and mean free path of HeII ionizing photons at : Evidence for late and rapid HeII reionization Part-II
arXiv:2503.04893 · doi:10.1088/1475-7516/2025/09/057
Abstract
We present measurements of the spatially averaged HeII photo-ionization rate (), mean free path of HeII ionizing photons (), and HeII fraction () across seven redshift bins within the redshift range . The measurements are obtained by comparing the observed effective optical depth distribution of HeII () with models generated by post-processing of the Sherwood simulation suite using our code EXCITE. With EXCITE, we efficiently explore a large parameter space ( models) by varying and . We employ Anderson-Darling test for the cumulative distribution of to simultaneously measure and . Our measurements account for possible observational and modeling uncertainties stemming mainly from the finite signal-to-noise ratio of the observed data and thermal parameter uncertainties. We find significant evolution, with the best-fit and decreasing by factors of and , respectively, from to . Based on these measurements, we constrain the emissivity at the HeII ionization frequency () and HeII ionizing photon emission rate (), finding consistency with results from galaxy and QSO surveys. Comparison of our measured parameters with widely used uniform UVB models supports a scenario where HeII reionization is not completed before . Our measured evolution is complementary and in good agreement with recent measurements of thermal parameters of the IGM, suggesting a coherent picture of rather late and rapid HeII reionization.
arXiv comment39 pages, 14 figures, 2 tables; Published in JCAP; Main results are summarized in Fig. 7, Fig. 8 and Table 2
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