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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Mualliflar

A. C. Cobos Cerutti

Soʻnggi maʼlum muassasa:
National Scientific and Technical Research Council
ORCID:
0000-0002-0652-5460
4
h-indeks
0
i10-indeksi
36
Iqtiboslar
16
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013450510152020192020202120222024202520262019: Nashrlar 1, Iqtiboslar 02020: Nashrlar 1, Iqtiboslar 02021: Nashrlar 2, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 52024: Nashrlar 1, Iqtiboslar 62025: Nashrlar 5, Iqtiboslar 192026: Nashrlar 4, Iqtiboslar 6

Iqtibos tarixi

0510152020192020202120222024202520262019: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 52024: Iqtiboslar 62025: Iqtiboslar 192026: Iqtiboslar 6

Nashr tarixi

0134520192020202120222024202520262019: Nashrlar 12020: Nashrlar 12021: Nashrlar 22022: Nashrlar 22024: Nashrlar 12025: Nashrlar 52026: Nashrlar 4

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520192020202120222024202520262019: h-indeks 02020: h-indeks 02021: h-indeks 02022: h-indeks 12024: h-indeks 22025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. 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
  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. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  7. The Pierre Auger Observatory open data20250 iqtibos
  8. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 iqtibos
  9. Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory20260 iqtibos
  10. Long-term monitoring of the optical performance of the primary mirrors at the Coihueco and Loma Amarilla sites of the Pierre Auger Observatory20260 iqtibos

Hammualliflar

Yana 12 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 4 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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