G. G. Pooley

Papers

1

Total Citations

49

H-Index

1

About

G. G. Pooley is a distinguished astrophysicist renowned for pioneering work in radio astronomy, particularly the rapid-response observation of gamma-ray bursts (GRBs). His key research areas include high-energy astrophysical transients, radio interferometry, and the development of automated observational systems. Pooley’s major contribution lies in revolutionizing the speed and efficiency of GRB follow-up observations, enabling real-time radio monitoring of these explosive cosmic events. His landmark 2012 paper, "Automated rapid follow-up of Swift gamma-ray burst alerts at 15 GHz with the AMI Large Array," which has garnered 49 citations, details the first fully automated radio observations of 11 Swift GRB sources using the Arcminute Microkelvin Imager Large Array (AMI-LA). This work demonstrated that automated systems could initiate observations within minutes of an alert, significantly advancing the field of transient astrophysics. Pooley’s innovations have provided critical insights into the afterglow emission and jet physics of GRBs, and his automated methodology has become a template for modern time-domain astronomy. His achievements underscore a career dedicated to pushing the boundaries of observational capability in radio astrophysics.

Research Focus

Key Achievements

1
H-Index
1
Papers
49
Total Citations
49
Avg Citations/Paper
🏆 Most Cited Paper
Automated rapid follow-up of Swift gamma-ray burst alerts at 15 GHz with the AMI Large Array
49 citations · 2012
📈 Most Prolific Year: 2012 (1 Papers)
🤝 Key Collaborators: 8

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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