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Mualliflar

G. Ávila

Soʻnggi maʼlum muassasa:
National Atomic Energy Commission
2
h-indeks
0
i10-indeksi
11
Iqtiboslar
8
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01345035810202020222024202520262020: Nashrlar 1, Iqtiboslar 02022: Nashrlar 0, Iqtiboslar 12024: Nashrlar 3, Iqtiboslar 02025: Nashrlar 4, Iqtiboslar 62026: Nashrlar 0, Iqtiboslar 4

Iqtibos tarixi

035810202020222024202520262020: Iqtiboslar 02022: Iqtiboslar 12024: Iqtiboslar 02025: Iqtiboslar 62026: Iqtiboslar 4

Nashr tarixi

01345202020222024202520262020: Nashrlar 12022: Nashrlar 02024: Nashrlar 32025: Nashrlar 42026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

012202020222024202520262020: h-indeks 02022: h-indeks 12024: h-indeks 12025: h-indeks 22026: h-indeks 2

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. 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
  3. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  6. Search for photons above <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>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory20240 iqtibos
  7. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  8. PLATOSpec: a precise spectrograph in support of space missions20250 iqtibos

Hammualliflar

  1. M. Roth1 ta umumiy asar2025
  2. V. D. Ivanov1 ta umumiy asar2025
  3. E. W. Guenther1 ta umumiy asar2025
  4. Martin Veselý1 ta umumiy asar2025
  5. Antonio Fuentes1 ta umumiy asar2025
  6. Jan Janík1 ta umumiy asar2025
  7. Marek Skarka1 ta umumiy asar2025
  8. H. M. J. Boffin1 ta umumiy asar2025
  9. J. Zak1 ta umumiy asar2025
  10. P. Kábath1 ta umumiy asar2025

Yana 7 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

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