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G. Ryan

4 papers here

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

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • G. Ryan — 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

most citedX-ray follow-up of extragalactic transients

2 citations · 2 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2019

Gamma-Ray Burst Afterglows In The Multi-Messenger Era: Numerical Models and Closure Relations

Geoffrey Ryan, Hendrik van Eerten, Luigi Piro +1

Gamma-ray bursts (GRBs) associated with gravitational wave events are, and will likely continue to be, viewed at a larger inclination than GRBs without gravitational wave detection…

astro-ph.HE2019

The afterglow and kilonova of the short GRB 160821B

E. Troja, A. J. Castro-Tirado, J. Becerra Gonzalez +22

GRB 160821B is a short duration gamma-ray burst (GRB) detected and localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z=0.1613, at a projected p…

astro-ph.HE2019★ 2 cited

X-ray follow-up of extragalactic transients

Erin Kara, Raffaella Margutti, Azadeh Keivani +11

Most violent and energetic processes in our universe, including mergers of compact objects, explosions of massive stars and extreme accretion events, produce copious amounts of X-r…

astro-ph.HE2018

A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations

L. Piro, E. Troja, B. Zhang +12

Multi-messenger observations of GW170817 have not conclusively established whether the merger remnant is a black hole (BH) or a neutron star (NS). We show that a long-lived magneti…

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