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researcher

A. Etchegoyen

96 papers hereh-index 5516.1k citations382 works total

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

author position
  • middle author18
  • last author7

Across the 25 of 96 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE50
  • astro-ph.IM32
  • astro-ph4
  • hep-ex4
  • hep-ph2
  • physics.ins-det2
same name
  • A. Etchegoyen — 13 papers, h 16
  • A. Etchegoyen — 12 papers
  • A. Etchegoyen — 3 papers
  • A. Etchegoyen — 2 papers, h 5
  • A. Etchegoyen — 1 paper, h 1
  • A. Etchegoyen — 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
20052026
most citedTesting Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

236 citations · 1.5k across the 60 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.HE2012★ 76 cited

Search for Point-Like Sources of Ultra-High Energy Neutrinos at the Pierre Auger Observatory and Improved Limit on the Diffuse Flux of Tau Neutrinos

Pierre Auger Collaboration

The Surface Detector array of the Pierre Auger Observatory can detect neutrinos with energy between 10^17 eV and 10^20 eV from point-like sources across the sky south of +55 deg an…

astro-ph.IM2012★ 148 cited

Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

P. Abreu, M. Aglietta, M. Ahlers +512

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineer…

astro-ph.IM2012★ 35 cited

The Rapid Atmospheric Monitoring System of the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +508

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10^17 eV. During clear nights with a low illuminated moon fraction, the UV fluo…

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