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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*†‡

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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 Click to show full abstract

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

Keywords: density; low density; flux column; column density; transmitted flux

Journal Title: Monthly Notices of the Royal Astronomical Society
Year Published: 2020

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