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researcher

T. Karlsson

18 papers hereh-index 141.3k citations31 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author6
  • middle author10

Across the 18 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph9
  • astro-ph.CO4
  • astro-ph.SR3
  • astro-ph.EP1
  • astro-ph.GA1
same name
  • T. Karlsson — 6 papers, h 31
  • T. Karlsson — 2 papers, h 3
  • T. Karlsson — 2 papers, h 5
  • T. Karlsson — 1 paper, h 9
  • T. Karlsson — 1 paper, h 2
  • T. Karlsson — 1 paper, h 10

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982025
most citedA stellar relic from the early Milky Way

527 citations · 1.6k across the 18 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2025★ 5 cited

Observations of UX Ori in deep minima with the Nordic Optical Telescope. I. Analysis of spectral lines

L. V. Tambovtseva, A. A. Djupvik, V. P. Grinin +11

UX Orionis stars are the most active young stars; they undergo sporadic fadings of 2 - 4 magnitudes in the V-band, due to variable circumstellar extinction caused by a nearly edge-…

astro-ph.SR2023★ 10 cited

Modelling UX Ori Star Eclipses based on Spectral Observations with the Nordic Optical Telescope. I. RR Tau

V. P. Grinin, L. V. Tambovtseva, A. A. Djupvik +12

Based on observations obtained with the Nordic Optical Telescope we investigate the spectral variability of the Herbig Ae star RR Tau. This star belongs to the UX Ori family, chara…

astro-ph.SR2010★ 23 cited

The Hamburg/ESO R-process Enhanced Star survey (HERES) VI. The Galactic Chemical Evolution of Silicon

L. Zhang, T. Karlsson, N. Christlieb +3

We determined the silicon abundances of 253 metal-poor stars in the metallicity range −4<[Fe/H]<−1.5, based on non-local thermodynamic equilibrium (NLTE) line formation…

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