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K. Wiersema

152 papers hereh-index 5610.7k citations309 works total

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

author position
  • sole author2
  • first author8
  • middle author77
  • last author33

Across the 120 of 152 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE72
  • astro-ph25
  • astro-ph.GA19
  • astro-ph.CO15
  • astro-ph.IM9
  • astro-ph.SR9
same name
  • K. Wiersema — 41 papers, h 14
  • K. Wiersema — 13 papers, h 10
  • K. Wiersema — 9 papers, h 2
  • K. Wiersema — 8 papers
  • K. Wiersema — 5 papers, h 1
  • K. Wiersema — 1 paper, h 2

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
20052025
most citedMethods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

1.8k citations · 11.8k across the 152 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005★ 121 cited

A log N(HI) = 22.6 DLA in a dark gamma-ray burst: the environment of GRB 050401

D. Watson, J. P. U. Fynbo, C. Ledoux +33

The optical afterglow spectrum of GRB050401 (at z=2.8992+/-0.0004) shows the presence of a DLA, with log(nHI)=22.6+/-0.3. This is the highest column density ever observed in a DLA,…

astro-ph2005★ 85 cited

Gas and dust properties in the afterglow spectra of GRB 050730

R. L. C. Starling, P. M. Vreeswijk, S. L. Ellison +9

We present early WHT ISIS optical spectroscopy of the afterglow of gamma-ray burst GRB 050730. The spectrum shows a DLA system with the highest measured hydrogen column to date: N(…

astro-ph2005★ 3 cited

The search for the host galaxy of the gamma-ray burst GRB 000214

S. Guziy, J. Gorosabel, A. J. Castro-Tirado +7

We present UBVRI-band observations taken ~300 days after the BeppoSAX gamma-ray burst GRB 000214. This GRB did not show a detectable optical afterglow, however due to the localizat…

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