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Mualliflar

Juan Ammerman Yebra

Ism variantlari: J. Ammerman Yebra

Soʻnggi maʼlum muassasa:
University of Santiago de Compostela
ORCID:
0000-0002-2059-6206
3
h-indeks
0
i10-indeksi
42
Iqtiboslar
42
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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0613192505101520202220232024202520262022: Nashrlar 2, Iqtiboslar 02023: Nashrlar 9, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 24, Iqtiboslar 202026: Nashrlar 3, Iqtiboslar 11

Iqtibos tarixi

05101520202220232024202520262022: Iqtiboslar 02023: Iqtiboslar 02024: Iqtiboslar 112025: Iqtiboslar 202026: Iqtiboslar 11

Nashr tarixi

06131925202220232024202520262022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 242026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

01345202220232024202520262022: h-indeks 02023: h-indeks 02024: h-indeks 22025: h-indeks 22026: h-indeks 3

Eng koʻp iqtibos qilingan asarlar

  1. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory20243 iqtibos
  2. Inference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning20253 iqtibos
  3. Measurement of the depth of maximum of air-shower profiles with energies between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>20</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> using the surface detector of the Pierre Auger Observatory and deep learning20253 iqtibos
  4. Energy Spectrum of Ultrahigh-Energy Cosmic Rays across Declinations <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>−</mml:mo> <mml:mn>9</mml:mn> <mml:mn>0</mml:mn> <mml:mi>°</mml:mi> </mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>+</mml:mo> <mml:mn>44.8</mml:mn> <mml:mi>°</mml:mi> </mml:math> as Measured at the Pierre Auger Observatory20252 iqtibos
  5. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  6. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  7. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  8. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  9. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
  10. AugerPrime: Status and first results20251 iqtibos

Hammualliflar

  1. L. Nellen4 ta umumiy asar2025
  2. R. Ulrich4 ta umumiy asar2025
  3. J. Albrecht4 ta umumiy asar2025
  4. A. A. Alves4 ta umumiy asar2025
  5. Dominik Baack4 ta umumiy asar2025
  6. W. Rhode4 ta umumiy asar2025
  7. T. Huege4 ta umumiy asar2025
  8. Jean-Marco Alameddine4 ta umumiy asar2025
  9. Luisa Arrabito4 ta umumiy asar2025
  10. Cosmin Deaconu4 ta umumiy asar2025

Yana 28 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 10 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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