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researcher

C. Thöne

54 papers hereh-index 154.8k citations96 works total

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

author position
  • first author4
  • middle author41
  • last author2

Across the 47 of 54 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE30
  • astro-ph7
  • astro-ph.CO7
  • astro-ph.GA6
  • astro-ph.EP2
  • astro-ph.IM1
same name
  • C. Thöne — 37 papers, h 41

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
20062026
most citedGRB 090423 at a redshift of z~8.1

498 citations · 5k across the 53 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014

A young stellar environment for the superluminous supernova PTF12dam

C. C. Thöne, A. de Ugarte Postigo, R. García-Benito +3

The progenitors of super luminous supernovae (SLSNe) are still a mystery. Hydrogen-poor SLSN hosts are often highly star-forming dwarf galaxies and the majority belongs to the clas…

astro-ph.GA2014★ 55 cited

The mysterious optical afterglow spectrum of GRB140506A at z=0.889

J. P. U. Fynbo, T. Krühler, K. Leighly +40

Context. Gamma-ray burst (GRBs) afterglows probe sightlines to star-forming regions in distant star-forming galaxies. Here we present a study of the peculiar afterglow spectrum of…

astro-ph.GA2014★ 225 cited

Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies

G. Leloudas, S. Schulze, T. Kruehler +16

Superluminous supernovae (SLSNe) are very bright explosions that were only discovered recently and that show a preference for occurring in faint dwarf galaxies. Understanding why s…

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