J. A. Aguilar

University of Wisconsin–Madison

Papers

1

Total Citations

57

H-Index

1

About

J. A. Aguilar is a leading figure in astroparticle physics, whose research centers on the search for high-energy neutrino emissions from transient astrophysical phenomena. His work bridges the gap between multimessenger astronomy and neutrino detection, with a particular focus on core-collapse supernovae and gamma-ray bursts. Aguilar’s major contribution lies in developing and executing observational strategies to identify soft relativistic jets—less energetic than those in GRBs—that may accompany supernova explosions. In his highly cited 2012 study (57 citations), he detailed the IceCube optical follow-up program, which linked neutrino alerts to electromagnetic observations, enabling the search for transient neutrino sources on timescales of ~100 seconds. This work demonstrated how neutrino telescopes can probe the innermost engines of stellar explosions. Aguilar’s impact extends through his role in the IceCube Collaboration, where his efforts have advanced the understanding of non-thermal processes in the universe. His research remains pivotal for students and researchers exploring the connection between gravitational waves, neutrinos, and cosmic cataclysms.

Research Focus

Key Achievements

1
H-Index
1
Papers
57
Total Citations
57
Avg Citations/Paper
🏆 Most Cited Paper
Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program
57 citations · 2012
📈 Most Prolific Year: 2012 (1 Papers)
🤝 Key Collaborators: 98
🏛 Institutions: University of Wisconsin–Madison

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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