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Kim K. Nilsson

Researcher at European Southern Observatory

Publications -  30
Citations -  2061

Kim K. Nilsson is an academic researcher from European Southern Observatory. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 20, co-authored 30 publications receiving 1884 citations. Previous affiliations of Kim K. Nilsson include Niels Bohr Institute & University of Copenhagen.

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Evolution in the properties of Lyman-alpha emitters from redshifts z ~ 3 to z ~ 2

TL;DR: In this article, the authors studied the properties of 2.25 LAEs and compared them with those of z > 3 LAEs, showing that there has been significant evolution in LAEs between redshift z = 3 and z = 2.5.
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A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo

TL;DR: In this paper, it was shown that the most probable origin of the extended Ly-alpha emission from the blob in the GOODS South field is cold accretion onto a dark matter halo.
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A multi-wavelength study of z = 3.15 Lyman-alpha emitters in the GOODS South Field

TL;DR: In this paper, the spectral energy distribution of Lyman break galaxies is studied at the 4 sigma level, and it is shown that the rest-frame UV SED of these galaxies is very similar to that of LBGs and comply with the selection criteria for U-band drop-out, except they are intrinsically fainter than the current limit for LBGs.
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Mass–metallicity relation from z = 5 to the present: evidence for a transition in the mode of galaxy growth at z = 2.6 due to the end of sustained primordial gas infall

TL;DR: This article analyzed the redshift evolution of the mass-metallicity relation in a sample of 110 Damped Ly$\alpha$ absorbers and found that the zero-point of the correlation changes significantly with redshift.