D. J. Sullivan

Victoria University of Wellington

Papers

1

Total Citations

25

H-Index

1

About

D. J. Sullivan is a leading figure in astrophysics, specializing in gravitational microlensing and exoplanet detection. His research focuses on the development of automated real-time systems to identify subtle anomalies in stellar light curves, enabling the discovery of low-mass objects such as brown dwarfs and exoplanets. Sullivan’s major contribution includes the first automated real-time detection of a weak microlensing anomaly, detailed in his 2012 study of OGLE-2008-BLG-510. This work demonstrated the power of the Automated Robotic Terrestrial Exoplanet Microlensing Search (ARTEMiS) system, which promptly identified an asymmetric light curve peak, distinguishing between a brown dwarf and a stellar binary. With 25 citations, this paper highlights his impact on advancing rapid-response observational techniques. Sullivan’s achievements have paved the way for more efficient exoplanet surveys, influencing both robotic telescope automation and the interpretation of microlensing events. His work remains essential for researchers exploring the frontiers of planetary and stellar astrophysics.

Research Focus

Key Achievements

1
H-Index
1
Papers
25
Total Citations
25
Avg Citations/Paper
🏆 Most Cited Paper
OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly - brown dwarf or stellar binary?★
25 citations · 2012
📈 Most Prolific Year: 2012 (1 Papers)
🤝 Key Collaborators: 98
🏛 Institutions: Victoria University of Wellington

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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