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researcher

H. Fausey

15 papers hereh-index 6102 citations17 works total

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

author position
  • first author4
  • middle author8
  • last author1

Across the 13 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE7
  • astro-ph.IM3
  • astro-ph.CO2
  • astro-ph.EP1
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • H. Fausey — 1 paper

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
20182026
most citedDissecting the interstellar medium of a z=6.3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A

33 citations · 117 across the 12 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.HE2025

The radio flare and multi-wavelength afterglow of the short GRB 231117A: energy injection from a violent shell collision

G. E. Anderson, G. P. Lamb, B. P. Gompertz +64

We present the early radio detection and multi-wavelength modeling of the short gamma-ray burst (GRB) 231117A at redshift z=0.257. The Australia Telescope Compact Array automatic…

astro-ph.HE2025★ 2 cited

JWST reveals a supernova following a gamma-ray burst at z ≃ 7.3

A. J. Levan, B. Schneider, E. Le Floc'h +50

The majority of energetic long-duration gamma-ray bursts (GRBs) are thought to arise from the collapse of massive stars, making them powerful tracers of star formation across cosmi…

astro-ph.HE2025

SVOM GRB 250314A at z ≃ 7.3: an exploding star in the era of reionization

B. Cordier, J. Y. Wei, N. R. Tanvir +103

Most long Gamma-ray bursts originate from a rare type of massive stellar explosion. Their afterglows, while rapidly fading, can be initially extremely luminous at optical/near-infr…

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