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Smith, A. J.

  1. Science Case for a Wide Field-of-View Very-High-Energy Gamma-Ray Observatory in the Southern Hemisphere
    2019/02/22 by Albert, A., Alfaro, R., Ashkar, H. +100 · 6 citations
    #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM)
  2. Galactic Gamma-Ray Diffuse Emission at TeV energies with HAWC Data
    2023/10/13 by R. Alfaro, C. Álvarez, Alfaro, R. +156 · 8 citations
    Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Particle Detector Development and Performance
  3. The Future Of The Arecibo Observatory: The Next Generation Arecibo Telescope
    2021/03/02 by D. Anish Roshi, N. Aponte, Roshi, D. Anish +145 · 1 voice · 1 citation
    #astro-ph.IM #astro-ph.EP #astro-ph.SR #physics.ao-ph #physics.ins-det
  4. Performance of the HAWC Observatory and TeV Gamma-Ray Measurements of the Crab Nebula with Improved Extensive Air Shower Reconstruction Algorithms
    2024/05/09 by A. Albert, R. Alfaro, Albert, A . +182 · 6 citations
    Computer Science · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Computational Physics and Python Applications #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Radio Astronomy Observations and Technology
  5. Calibration of the Milagro Cosmic Ray Telescope
    1999/06/25 by R. Atkins, W. Benbow, Atkins, R. +91 · 1 citation
    Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Particle Detector Development and Performance #Radiation Detection and Scintillator Technologies #astro-ph
  6. Observation of the Galactic Center PeVatron Beyond 100 TeV with HAWC
    2024/07/04 by Albert, A., Alfaro, R., Alvarez, C. +99 · 3 citations
    #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE)
  7. Science Prospects for the Southern Wide-field Gamma-ray Observatory: SWGO
    2025/06/02 by Swgo Collaboration, P. Abreu, SWGO Collaboration +396 · 5 citations
    Physics and Astronomy · #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Gamma-ray bursts and supernovae #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Particle Detector Development and Performance
  8. High Altitude characterization of the Hunga Pressure Wave with Cosmic Rays by the HAWC Observatory
    2022/09/29 by R. Alfaro, Alfaro, R., C. Alvarez +131 · 1 citation
    Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Experiment (hep-ex) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Neutrino Physics Research
  9. Limits on the Diffuse Gamma-Ray Background above 10 TeV with HAWC
    2022/09/16 by HAWC Collaboration, Albert, A., Alfaro, R. +87 · 1 citation
    #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE)
  10. Uncertainty quantification in (p,n) reactions
    2024/03/27 by A. J. Smith, Smith, A. J., C. Hebborn +5 · 1 citation
    Decision Sciences · Mathematics · #FOS: Physical sciences #Nuclear Experiment (nucl-ex) #Nuclear Theory (nucl-th) #Probabilistic and Robust Engineering Design #Statistical Distribution Estimation and Applications #Statistical Methods and Inference
  11. TeV Analysis of a Source Rich Region with HAWC Observatory: Is HESS J1809-193 a Potential Hadronic PeVatron?
    2024/07/11 by A. Albert, R. Alfaro, Albert, A. +161 · 1 citation
    Physics and Astronomy · Engineering · #Astrophysics and Cosmic Phenomena #Astronomical Observations and Instrumentation #Particle Accelerators and Free-Electron Lasers
  12. Orbital Modulation of Gamma-Rays Beyond 100 TeV from LS 5039
    2025/03/26 by Alfaro, R., Araya, M., Arteaga-Velázquez, J. C. +88 · 1 citation
    #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE)