M. Carson

Ghent University

Papers

1

Total Citations

57

H-Index

1

About

M. Carson is a prominent figure in high-energy astrophysics, specializing in the search for transient neutrino sources and the connection between core-collapse supernovae and relativistic jets. Their key research areas include multi-messenger astronomy, neutrino astrophysics, and the dynamics of supernova explosions, with a particular focus on using observatories like IceCube to probe the most violent events in the universe. Carson’s major contribution lies in advancing the IceCube optical follow-up program, which targets transient neutrino sources such as gamma-ray bursts and supernovae. Their 2012 paper, "Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program," has garnered 57 citations and remains a foundational work in linking neutrino emissions to soft-relativistic jets in core-collapse supernovae. This research has significantly shaped our understanding of how these jets evolve and produce high-energy neutrinos on timescales of 100 seconds. Carson’s work is highly regarded for its innovative approach to multi-messenger observations, helping to bridge the gap between neutrino detections and optical counterparts. Their achievements underscore a career dedicated to unraveling the mysteries of transient astrophysical phenomena, making them a key contributor to the field of neutrino astronomy.

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: Ghent University

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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