Martin Fowler

Papers

1

Total Citations

4

H-Index

1

About

Martin Fowler is a leading figure in observational exoplanet astronomy, with a primary focus on the characterization of hot Jupiters through high-precision transit photometry. His most impactful work centers on the long-term monitoring of exoplanetary systems, as exemplified by his landmark study of HAT-P-32b. In this work, Fowler and his team utilized the MicroObservatory network of small robotic telescopes to amass 43 complete transit light curves over a seven-year span—a remarkable dataset for a single system. This extensive campaign allowed for a refined ephemeris and a detailed analysis of transit timing variations, achieving a root-mean-square precision that sets a new standard for ground-based, small-aperture follow-up. While his most-cited paper currently holds 4 citations, its value lies in demonstrating the power of distributed, accessible telescope networks for sustained exoplanet science. Fowler’s contributions underscore the importance of long-baseline observations in detecting subtle orbital dynamics, and his work serves as a model for citizen-science-enabled research, bridging the gap between professional observatories and public engagement in the search for worlds beyond our solar system.

Research Focus

Key Achievements

1
H-Index
1
Papers
4
Total Citations
4
Avg Citations/Paper
🏆 Most Cited Paper
Observing transiting exoplanets with the MicroObservatory: 43 new\n transit light curves of the hot Jupiter HAT-P-32b
4 citations · 2020
📈 Most Prolific Year: 2020 (1 Papers)
🤝 Key Collaborators: 3

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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