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The evolution of the low-density H i  intergalactic medium from z = 3.6 to 0: Data, transmitted flux and H i column density*†‡
Monthly Notices of the Royal Astronomical Society ( IF 4.7 ) Pub Date : 2020-12-14 , DOI: 10.1093/mnras/staa3844
T-S Kim 1, 2 , B P Wakker 1 , F Nasir 3, 4 , R F Carswell 5 , B D Savage 1 , J S Bolton 3 , A J Fox 6 , M Viel 2, 7, 8, 9 , M G Haehnelt 5 , J C Charlton 10 , B E Rosenwasser 1
Affiliation  

We present a new, uniform analysis of the HI transmitted flux (F) and HI column density (N(HI)) distribution in the low-density IGM as a function of redshift z for 0

中文翻译:

低密度 H i 星系际介质从 z = 3.6 到 0 的演变:数据、传输通量和 H i 柱密度*†‡

我们对低密度 IGM 中的 HI 透射通量 (F) 和 HI 柱密度 (N(HI)) 分布进行了新的、统一的分析,作为 0 时红移 z 的函数
更新日期:2020-12-14
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