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Antonio Condorelli

Soʻnggi maʼlum muassasa:
Université Paris-Saclay
ORCID:
0000-0001-5681-0086
4
h-indeks
0
i10-indeksi
68
Iqtiboslar
26
Asarlar
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01325385020192020202120222023202420252019: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 02023: Iqtiboslar 02024: Iqtiboslar 182025: Iqtiboslar 50

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03581020192020202120222023202420252019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 72024: Nashrlar 22025: Nashrlar 2

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0134520192020202120222023202420252019: h-indeks 02020: h-indeks 02021: h-indeks 02022: h-indeks 02023: h-indeks 02024: h-indeks 22025: h-indeks 4

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
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