Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: Monte Carlo simulations for the Pierre Auger Observatory using the VO auger grid resources

1. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory

   Adila Abdul Halim, P. Abreu, M. Aglietta +96

   МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20242 иқтибос

   ABIABI:AkademIndex/openalex/2024.article.000207

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 Learning

   Adila Abdul Halim, P. Abreu, M. Aglietta +97

   МақолаAstrophysics and Cosmic PhenomenaPhysical Review Letters20252 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.000110

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 learning

   Adila Abdul Halim, P. Abreu, M. Aglietta +97

   МақолаAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20252 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.111785