Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
[At the AAS,] All the talks I attended were truly interesting. It is pleasure to have others teach me!
In its current form, anyone with moderate computer skills and high school physics can download, explore, and begin to understand available data.
[Because of a poster I saw at the AAS and] my participation in the NITARP program, I will be raising the standards for my students in the future.
