Industrial University of Santander

Eng koʻp iqtibos qilingan asarlar

1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 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. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
4. Study of the leptonic decays of the Z0 boson19902 iqtibos
5. A measurement of the tau lifetime19931 iqtibos
6. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
7. Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory20260 iqtibos
8. Long-term monitoring of the optical performance of the primary mirrors at the Coihueco and Loma Amarilla sites of the Pierre Auger Observatory20260 iqtibos
9. Depth of maximum of air-shower profiles above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msup> <mml:mn>10</mml:mn> <mml:mn>17.7</mml:mn> </mml:msup> <mml:mtext> </mml:mtext> <mml:mtext> </mml:mtext> <mml:mi>eV</mml:mi> </mml:math> measured with the fluorescence detector of the Pierre Auger Observatory20260 iqtibos
10. Bounds on Lorentz Invariance Violation from Muon Fluctuations at the Pierre Auger Observatory20260 iqtibos