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researcher

G. Stratta

85 papers hereh-index 7532.1k citations396 works total

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

author position
  • first author9
  • middle author45
  • last author12

Across the 66 of 85 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE35
  • astro-ph23
  • astro-ph.IM14
  • gr-qc7
  • astro-ph.CO6
same name
  • G. Stratta — 52 papers
  • G. Stratta — 33 papers, h 17
  • G. Stratta — 2 papers, h 15
  • G. Stratta — 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
19992026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 4.6k across the 82 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005

INTEGRAL observation of the X-ray burster KS 1741-293

G. De Cesare, A. Bazzano, G. Stratta +3

KS 1741-293 was firstly detected in 1989 with the X-ray wide field camera TTM (3-10 keV) on board of the Rontgen-Kvant-Mir observatory. During these observations this source exhibi…

astro-ph2005

GRB environment properties through X and optical afterglow observations

M. L Conciatore, L. A. Antonelli, G. Stratta +2

We present the spectral analysis of 14 gamma-ray bursts (GRB) X-ray afterglows in order to investigate the properties of interstellar matter (ISM) along the line of sight of GRB. W…

astro-ph2005★ 43 cited

Extinction properties of the X-ray bright/optically faint afterglow of GRB 020405

G. Stratta, R. Perna, D. Lazzati +3

We present an optical-to-X-ray spectral analysis of the afterglow of GRB 020405. The optical spectral energy distribution not corrected for the extragalactic extinction is signific…

astro-ph2005★ 39 cited

Early re-brightening of the afterglow of GRB 050525a

A. Klotz, M. Boer, J. L. Atteia +4

We present time resolved optical data acquired by the TAROT automated observatory on the afterglow of GRB 050525a from 6 to 136 minutes after the GRB. We evidence a rapid re-bright…

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