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researcher

G. Fontaine

115 papers hereh-index 328.5k citations160 works total

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

author position
  • middle author17
  • last author1

Across the 18 of 115 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE64
  • astro-ph33
  • astro-ph.IM14
  • astro-ph.CO2
  • astro-ph.GA1
  • hep-ex1
same name
  • G. Fontaine — 152 papers, h 78
  • G. Fontaine — 44 papers, h 11
  • G. Fontaine — 30 papers, h 23
  • G. Fontaine — 29 papers
  • G. Fontaine — 3 papers, h 2
  • G. Fontaine — 3 papers, h 11

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
20042023
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 9.5k across the 113 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.IM2016★ 15 cited

NectarCAM, a camera for the medium sized telescopes of the Cherenkov Telescope Array

J-F. Glicenstein, M. Shayduk

NectarCAM is a camera proposed for the medium-sized telescopes of the Cherenkov Telescope Array (CTA) which covers the core energy range of ~100 GeV to ~30 TeV. It has a modular de…

astro-ph.HE2016★ 29 cited

Introduction to high-energy gamma-ray astronomy

Bernard Degrange, Gérard Fontaine

The present issue is the first of of a two-volume review devoted to gamma-ray astronomy above 100 MeV which has witnessed considerable progress over the last 20 years. The motivati…

astro-ph.HE2016★ 512 cited

Acceleration of petaelectronvolt protons in the Galactic Centre

H. E. S. S. collaboration, :, A. Abramowski +229

Galactic cosmic rays reach energies of at least a few Peta-electronvolts (1 PeV =1015 electron volts). This implies our Galaxy contains PeV accelerators (PeVatrons), bu…

astro-ph.HE2016★ 30 cited

Detailed spectral and morphological analysis of the shell type SNR RCW 86

H. E. S. S. Collaboration, A. Abramowski, F. Aharonian +232

Aims: We aim for an understanding of the morphological and spectral properties of the supernova remnant RCW~86 and for insights into the production mechanism leading to the RCW~86…

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