Kévin Almeida Cheminant
Ism variantlari: K. Almeida Cheminant
- Soʻnggi maʼlum muassasa:
- National Institute for Subatomic Physics
- ORCID:
- 0000-0001-6352-5339
3
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42
Iqtiboslar
39
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- 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
- 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
- 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
- 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
- A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
- Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
- Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
- A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
- Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
- AugerPrime: Status and first results20251 iqtibos
Hammualliflar
- H. Wilczyński1 ta umumiy asar2023
- M. Roth1 ta umumiy asar2023
- Jarosław Stasielak1 ta umumiy asar2023
- D. Góra1 ta umumiy asar2023
- R. Engel1 ta umumiy asar2023
- T. Pierog1 ta umumiy asar2023
- Jan Pękala1 ta umumiy asar2023
- M. Unger1 ta umumiy asar2023
- Darko Veberič1 ta umumiy asar2023
- Nataliia Borodai1 ta umumiy asar2023
Yana 28 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan
Skelet yozuvlar: 10 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan