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.
It was wonderful to see the students from last year presenting their posters and talking with astronomers and teachers from all over the world.
The most interesting thing I learned was that it is possible for very young students to wrap their heads around complex “higher level” science if they are motivated and engaged.
I already have more energy in the classroom and feel the need to pinch myself constantly.
