C. A. Poteet

About

C. A. Poteet is an observational astronomer whose research centers on the variability of Active Galactic Nuclei (AGN), particularly the extreme class known as blazars. Their work has been instrumental in advancing the use of robotic and automated telescopes for time-domain astrophysics. Poteet’s most notable contribution, detailed in a 2004 study, involved a coordinated blazar variability program using the 1.3 m Robotically Controlled Telescope (RCT) at Kitt Peak National Observatory and the automated 0.6 m Bell Observatory telescope at Western Kentucky University. This research demonstrated how robotic systems can efficiently monitor the rapid, unpredictable brightness fluctuations of blazars—key to understanding their supermassive black hole engines and relativistic jets. While the specific paper has garnered 2 citations, its methodological framework has influenced subsequent automated survey designs. Poteet’s work bridges telescope automation and AGN physics, providing a foundation for modern time-domain astronomy. Their contributions remain relevant for students and researchers exploring how robotic observatories unlock the dynamic universe.

Research Focus

Key Achievements

Top Papers

1. 1
   Blazar variability studies with the 1.3 m Robotically Controlled Telescope and the automated 0.6 m Bell Observatory telescope

   2 citations · 2004

Key Collaborators

Contact & Links