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F. Catalani

Ism variantlari: Fernando Catalani

Soʻnggi maʼlum muassasa:
University of São Paulo
ORCID:
0000-0001-9332-1476
4
h-indeks
0
i10-indeksi
74
Iqtiboslar
45
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
051015200132538502018201920202021202220232024202520262018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 22020: Nashrlar 3, Iqtiboslar 12021: Nashrlar 5, Iqtiboslar 02022: Nashrlar 1, Iqtiboslar 102023: Nashrlar 7, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 20, Iqtiboslar 372026: Nashrlar 3, Iqtiboslar 13

Iqtibos tarixi

0132538502018201920202021202220232024202520262018: Iqtiboslar 02019: Iqtiboslar 22020: Iqtiboslar 12021: Iqtiboslar 02022: Iqtiboslar 102023: Iqtiboslar 02024: Iqtiboslar 112025: Iqtiboslar 372026: Iqtiboslar 13

Nashr tarixi

051015202018201920202021202220232024202520262018: Nashrlar 12019: Nashrlar 12020: Nashrlar 32021: Nashrlar 52022: Nashrlar 12023: Nashrlar 72024: Nashrlar 42025: Nashrlar 202026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

013452018201920202021202220232024202520262018: h-indeks 02019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 22023: h-indeks 22024: 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. 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
  4. 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
  5. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  6. 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
  7. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  9. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  10. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos

Hammualliflar

Yana 29 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 16 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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