The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low-ℓ CMB

The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low-ℓ CMBDOI: info:10.1093/mnras/stab2815v. 5082784–2797
Wu, Xiaohan, McQuinn, Matthew, Eisenstein, Daniel, and Iršič, Vid. 2021. "The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low-ℓ CMB." Monthly Notices of the Royal Astronomical Society, 508 2784–2797. https://doi.org/10.1093/mnras/stab2815.
ID: 163601
Type: article
Keywords: SAO