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Nature|August 14, 2024
Origin and evolution of the bread wheat D genomeEmile Cavalet-Giorsa, Andrea González-Muñoz, Naveenkumar Athiyannan, et al.Physical Review Letters|December 23, 2022
Observation of a Strongly Isospin-Mixed Doublet in ^{26}Si via β-Delayed Two-Proton Decay of ^{26}PJ J Liu, X X Xu, L J Sun, et al.Physical Review Letters|February 25, 2022
Multidimensional, High Precision Measurements of Beam Single Spin Asymmetries in Semi-inclusive π^{+} Electroproduction off Protons in the Valence RegionS Diehl, A Kim, G Angelini, et al.Physical Review Letters|December 11, 2014
Precision Measurement of the (e^{+}+e^{-}) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space StationM Aguilar, D Aisa, B Alpat, et al.Physical Review Letters|October 4, 2014
Electron and positron fluxes in primary cosmic rays measured with the alpha magnetic spectrometer on the international space stationM Aguilar, D Aisa, A Alvino, et al.Physical Review Letters|October 4, 2014
High statistics measurement of the positron fraction in primary cosmic rays of 0.5-500 GeV with the alpha magnetic spectrometer on the international space stationL Accardo, M Aguilar, D Aisa, et al.Physical Review Letters|December 5, 2015
Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Magnetic Spectrometer on the International Space StationM Aguilar, D Aisa, B Alpat, et al.Physical Review Letters|May 16, 2015
Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space StationM Aguilar, D Aisa, B Alpat, et al.Physical Review Letters|August 29, 2014
First result from the Alpha Magnetic Spectrometer on the International Space Station: precision measurement of the positron fraction in primary cosmic rays of 0.5-350 GeVM Aguilar, G Alberti, B Alpat, et al.Physical Review Letters|April 11, 2026
Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeVZhen Cao, F Aharonian, Y X Bai, et al.Pageof 184