M. Barbieri
Papers
1
Total Citations
31
H-Index
1
About
M. Barbieri is a leading figure in exoplanetary astronomy, specializing in the detection and characterization of transiting exoplanets, particularly those orbiting K-dwarf stars. Their most impactful work centers on the discovery and analysis of multi-planet systems near mean motion resonances, a key area for understanding planetary formation and orbital dynamics. Barbieri’s landmark 2021 study, cited 31 times, identified TOI-2202 b, a warm Jovian-mass planet with an 11.91-day orbit, using TESS Full Frame Images and follow-up observations with the CHAT robotic telescope. This work not only confirmed a new giant planet but also revealed a pair of warm giants near a 2:1 mean motion resonance, offering critical insights into resonant capture and migration processes. Barbieri’s contributions have significantly advanced our knowledge of exoplanet demographics and the architecture of compact multi-planet systems. Their research, combining space-based transit surveys with ground-based photometric follow-up, demonstrates a rigorous approach to exoplanet validation and characterization, making them a respected voice in the field.
Research Focus
Key Achievements
Top Papers
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