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researcher

J. Elliott

37 papers hereh-index 231.4k citations74 works total

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

author position
  • first author8
  • middle author25

Across the 33 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE25
  • astro-ph.GA6
  • astro-ph.CO4
  • astro-ph.IM2
same name
  • J. Elliott — 17 papers, h 8
  • J. Elliott — 10 papers, h 13
  • J. Elliott — 7 papers, h 9
  • J. Elliott — 7 papers, h 17
  • J. Elliott — 5 papers, h 44
  • J. Elliott — 4 papers, h 3

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
20112024
most citedA very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst

303 citations · 2k across the 37 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 33 cited

Probing dust-obscured star formation in the most massive Gamma-Ray Burst host galaxies

Jochen Greiner, Michal J. Michalowski, Sylvio Klose +15

Due to their relation to massive stars, long-duration gamma-ray bursts (GRBs) allow pinpointing star formation in galaxies independently of redshift, dust obscuration, or galaxy ma…

astro-ph.HE2016★ 53 cited

Highly Luminous Supernovae associated with Gamma-Ray Bursts I.: GRB 111209A/SN 2011kl in the Context of Stripped-Envelope and Superluminous Supernovae

D. A. Kann, P. Schady, F. E. Olivares +22

GRB 111209A, one of the longest Gamma-Ray Bursts (GRBs) ever observed, is linked to SN 2011kl, the most luminous GRB-Supernova (SN) detected so far, which shows evidence for being…

astro-ph.GA2016★ 25 cited

Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?

R. S. de Souza, M. L. L. Dantas, A. Krone-Martins +7

We developed a hierarchical Bayesian model (HBM) to investigate how the presence of Seyfert activity relates to their environment, herein represented by the galaxy cluster mass, $M…

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