Tae-Sun Kim

Associate Scientist

Email: .(JavaScript must be enabled to view this email address)
Ph: (608) 262-5994
Office: 6516 Sterling Hall

Research Interests:

Redshift evolution of the Intergalactic Medium (IGM) and the Circumgalactic Medium (CGM) at 0 < z < 4; Galactic outflows and their connection to the cosmic star formation rate and galaxy evolution; Intensity and shape of the UV background; UV and optical spectroscopic analysis



For Selected Refereed Journals:

Mongardi C., Vie M., D'Odorico V., Kim T.-S. et al. 2018, MNRAS, 478, 3266, Absorption systems at z~2 as a probe of the circumgalactic medium: a probabilistic approach

Savage B. D., Kim T.-S., Fox A. J., Massa D. et al. 2017, ApJS, 232, 25, Probing the outflowing multiphase gas ~1 kpc below the Galactic center

Kim T.-S., Carswell R. F., Mongardi C., Partl A. M.,  Muecket J. P., Barai P., & Cristiani S. 2016, MNRAS, 4567, 2005, Triple-ionized carbon associated with the low-density neutral hydrogen gas at 1.7 < z < 3.3: the integrated N(HI)-N(CIV) relation

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