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researcher

D. Guetta

121 papers hereh-index 364.7k citations187 works total

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

author position
  • sole author6
  • first author31
  • middle author57
  • last author17

Across the 111 of 121 papers where every author was matched, so the position is known.

fields
  • astro-ph49
  • astro-ph.HE47
  • hep-ph9
  • astro-ph.CO6
  • astro-ph.IM5
  • astro-ph.SR3
same name
  • D. Guetta — 16 papers
  • D. Guetta — 6 papers
  • D. Guetta — 5 papers, h 15
  • D. Guetta — 3 papers
  • D. Guetta — 1 paper
  • D. Guetta — 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
19962026
most citedGRB 090423 at a redshift of z~8.1

498 citations · 5.4k across the 113 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.HE2010★ 31 cited

The High Energy Budget Allocations in Shocks and GRB

David Eichler, Dafne Guetta, Martin Pohl

The statistical distribution of energies among particles responsible for long Gamma Ray Burst (GRB) emission is analyzed in light of recent results of the Fermi Observatory. The al…

astro-ph.HE2010★ 173 cited

GRB Afterglows with Energy Injection from a spinning down NS

Simone Dall'Osso, Giulia Stratta, Dafne Guetta +3

We investigate a model for the shallow decay phases of Gamma-ray Burst (GRB) afterglows discovered by Swift/XRT in the first hours following a GRB event. In the context of the fire…

astro-ph.HE2010★ 41 cited

FERMI constraints on the high energy, ~1 GeV, emission of long GRBs

Dafne Guetta, Elena Pian, Eli Waxman

We investigate the constraints imposed on the luminosity function (LF) of long duration Gamma Ray Bursts (LGRBs) by the flux distribution of bursts detected by the GBM at ~1 MeV, a…

astro-ph.HE2010★ 4 cited

Wide Angle X-ray Sky Monitoring for Corroborating non-Electromagnetic Cosmic Transients

Dafne Guetta, David Eichler

Gravitational waves (GW) can be emitted from coalescing neutron star (NS) and black hole-neutron star (BH-NS) binaries, which are thought to be the sources of short hard gamma ray…

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