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Kévin Almeida Cheminant

Ism variantlari: K. Almeida Cheminant

Soʻnggi maʼlum muassasa:
National Institute for Subatomic Physics
ORCID:
0000-0001-6352-5339
3
h-indeks
0
i10-indeksi
42
Iqtiboslar
39
Asarlar
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0510152005101520202220232024202520262022: Nashrlar 2, Iqtiboslar 02023: Nashrlar 10, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 20, Iqtiboslar 202026: Nashrlar 3, Iqtiboslar 11

Iqtibos tarixi

05101520202220232024202520262022: Iqtiboslar 02023: Iqtiboslar 02024: Iqtiboslar 112025: Iqtiboslar 202026: Iqtiboslar 11

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05101520202220232024202520262022: Nashrlar 22023: Nashrlar 102024: Nashrlar 42025: Nashrlar 202026: Nashrlar 3

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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. 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
  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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  7. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  8. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  9. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
  10. AugerPrime: Status and first results20251 iqtibos
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