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F. Catalani

Ism variantlari: Fernando Catalani

Soʻnggi maʼlum muassasa:
Universidade de São Paulo
ORCID:
0000-0001-9332-1476
3
h-indeks
0
i10-indeksi
51
Iqtiboslar
29
Asarlar
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Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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0358100132538502018201920202021202220232024202520262018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 12020: Nashrlar 3, Iqtiboslar 12021: Nashrlar 5, Iqtiboslar 02022: Nashrlar 1, Iqtiboslar 12023: Nashrlar 7, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 6, Iqtiboslar 372026: Nashrlar 1, Iqtiboslar 0

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0132538502018201920202021202220232024202520262018: Iqtiboslar 02019: Iqtiboslar 12020: Iqtiboslar 12021: Iqtiboslar 02022: Iqtiboslar 12023: Iqtiboslar 02024: Iqtiboslar 112025: Iqtiboslar 372026: Iqtiboslar 0

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0358102018201920202021202220232024202520262018: Nashrlar 12019: Nashrlar 12020: Nashrlar 32021: Nashrlar 52022: Nashrlar 12023: Nashrlar 72024: Nashrlar 42025: Nashrlar 62026: Nashrlar 1

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013452018201920202021202220232024202520262018: h-indeks 02019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 12023: h-indeks 12024: h-indeks 22025: h-indeks 32026: 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 Observatory20242 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 Learning20252 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 learning20252 iqtibos
  4. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 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. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  8. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  9. The Pierre Auger Observatory open data20250 iqtibos
  10. 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 Observatory20250 iqtibos
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