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Ke Fang

Identifiers

  • name variant Ke Fang 0.60 · backfill

Papers (33)

  1. The Delta Resonance in the Neutrino Sky astro-ph.HE · 2026 · author #2
  2. MOSAIC: Module Discovery via Sparse Additive Identifiable Causal Learning for Scientific Time Series cs.LG · 2026 · author #4
  3. When and What to Ask: AskBench and Rubric-Guided RLVR for LLM Clarification cs.CL · 2026 · author #2
  4. The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios astro-ph.HE · 2025 · author #2
  5. Particle Astrophysics with High and Ultrahigh Energy Neutrinos astro-ph.HE · 2025 · author #1
  6. Search for synchrotron pair echo emission following KM3-230213A astro-ph.HE · 2025 · author #4
  7. IceCube Results and Perspective for Neutrinos from LHAASO Sources astro-ph.HE · 2024 · author #1
  8. Multimessenger Implications of AT2018cow: High-Energy Cosmic Ray and Neutrino Emissions from Magnetar-Powered Super-Luminous Transients astro-ph.HE · 2018 · author #1
  9. A Strong Test of the Dark Matter Origin of the 1.4 TeV DAMPE Signal Using IceCube Neutrinos astro-ph.HE · 2017 · author #2
  10. Double Neutron Star Mergers and Short Gamma-Ray Bursts: Long-Lasting High-Energy Signatures and Remnant Dichotomy astro-ph.HE · 2017 · author #3
  11. The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives astro-ph.IM · 2017 · author #1
  12. High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars astro-ph.HE · 2017 · author #1
  13. IceCube and HAWC constraints on very-high-energy emission from the Fermi bubbles astro-ph.HE · 2017 · author #1
  14. Using HAWC to Discover Invisible Pulsars astro-ph.HE · 2017 · author #5
  15. HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess astro-ph.HE · 2017 · author #4
  16. The Giant Radio Array for Neutrino Detection astro-ph.IM · 2017 · author #7
  17. The Highest-Energy Cosmic Rays Cannot be Dominantly Protons from Steady Sources astro-ph.HE · 2016 · author #1
  18. Identifying Ultrahigh-Energy Cosmic-Ray Accelerators with Future Ultrahigh-Energy Neutrino Detectors astro-ph.HE · 2016 · author #1
  19. High-energy neutrinos from sources in clusters of galaxies astro-ph.HE · 2016 · author #1
  20. Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy astro-ph.HE · 2016 · author #118
  21. A New Method for Finding Point Sources in High-energy Neutrino Data astro-ph.IM · 2016 · author #1
  22. IceCube Constraints on Fast-Spinning Pulsars as High-Energy Neutrino Sources astro-ph.HE · 2015 · author #1
  23. Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory astro-ph.HE · 2015 · author #118
  24. The Giant Radio Array for Neutrino Detection astro-ph.HE · 2015 · author #6
  25. Cluster Mergers and the Origin of the ARCADE-2 Excess astro-ph.HE · 2015 · author #1
  26. An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory astro-ph.HE · 2015 · author #121
  27. Measurement of the cosmic ray spectrum above $4{\times}10^{18}$ eV using inclined events detected with the Pierre Auger Observatory astro-ph.HE · 2015 · author #121
  28. The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation astro-ph.HE · 2014 · author #1
  29. High-Energy Neutrino Signatures of Newborn Pulsars In the Local Universe astro-ph.HE · 2014 · author #1
  30. Is the Ultra-High Energy Cosmic-Ray Excess Observed by the Telescope Array Correlated with IceCube Neutrinos? astro-ph.HE · 2014 · author #1
  31. Testing the Newborn Pulsar Origin of Ultrahigh Energy Cosmic Rays with EeV Neutrinos astro-ph.HE · 2013 · author #1
  32. Ultrahigh Energy Cosmic Ray Nuclei from Extragalactic Pulsars and the effect of their Galactic counterparts astro-ph.HE · 2013 · author #1
  33. Newly-born pulsars as sources of ultrahigh energy cosmic rays astro-ph.HE · 2012 · author #1

Mentions

  • 1511.08518 #1 · backfill · confidence 0.70 Ke Fang
  • 1508.04267 #118 · backfill · confidence 0.70 Ke Fang
  • 1508.01919 #6 · backfill · confidence 0.70 Ke Fang
  • 1506.05807 #1 · backfill · confidence 0.70 Ke Fang
  • 1504.05397 #121 · backfill · confidence 0.70 Ke Fang
  • 1503.07786 #121 · backfill · confidence 0.70 Ke Fang
  • 1412.7545 #1 · backfill · confidence 0.70 Ke Fang
  • 2606.00249 #2 · arxiv_oai · confidence 0.70 Ke Fang
  • 1411.2174 #1 · backfill · confidence 0.70 Ke Fang
  • 1404.6237 #1 · backfill · confidence 0.70 Ke Fang
  • 1311.2044 #1 · backfill · confidence 0.70 Ke Fang
  • 1302.4482 #1 · backfill · confidence 0.70 Ke Fang
  • 1201.5197 #1 · backfill · confidence 0.70 Ke Fang

Frequent Coauthors