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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 (2020)
Journal Article
Kim, T., Wakker, B. P., Nasir, F., Carswell, R. F., Savage, B. D., Bolton, J. S., …Rosenwasser, B. E. (2021). 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, 501(4), 5811-5833. https://doi.org/10.1093/mnras/staa3844

We present a new, uniform analysis of the H I transmitted flux (F) and H I column density (?NHI?) distribution in the low-density IGM as a function of redshift z for 0 < z < 3.6 using 55 HST/COS FUV (?z = 7.2 at z < 0.5), five HST/STIS+COS NUV (?z =... Read More about The evolution of the low-density H i intergalactic medium from z = 3.6 to 0: Data, transmitted flux, and H i column density.

Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Ly?forest spectra (2020)
Journal Article
Gaikwad, P., Rauch, M., Haehnelt, M. G., Puchwein, E., Bolton, J. S., Keating, L. C., …Rorai, A. (2020). Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Lyαforest spectra. Monthly Notices of the Royal Astronomical Society, 494(4), 5091–5109. https://doi.org/10.1093/mnras/staa907