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researcher

J. Kubát

52 papers hereh-index 17835 citations169 works total

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

author position
  • sole author5
  • first author3
  • middle author18
  • last author23

Across the 49 of 52 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR29
  • astro-ph20
  • hep-ex2
  • astro-ph.HE1
same name
  • J. Kubát — 50 papers, h 17
  • J. Kubát — 19 papers
  • J. Kubát — 7 papers, h 4
  • J. Kubát — 4 papers, h 5
  • J. Kubát — 3 papers, h 3
  • J. Kubát — 1 paper, h 0

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
20002026
most cited3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation

79 citations · 807 across the 52 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

hep-ex2021★ 14 cited

Study of the Bc+​ decays into charmonia and three light hadrons

LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb +996

Using proton-proton collision data, corresponding to an integrated luminosity of 9fb−1 collected with the LHCb detector, seven decay modes of the Bc+​ meson into a J/ψ or…

hep-ex2021★ 7 cited

Searches for rare Bs0​ and B0 decays into four muons

LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb +997

Searches for rare Bs0​ and B0 decays into four muons are performed using proton-proton collision data recorded by the LHCb experiment, corresponding to an integrated luminosi…

astro-ph.SR2021★ 33 cited

New mass-loss rates of B supergiants from global wind models

Jiri Krticka, Jiri Kubat, Iva Krtickova

Massive stars lose a significant fraction of mass during their evolution. However, the corresponding mass-loss rates are rather uncertain. To improve this, we calculated global lin…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.