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.
My skills and knowledge as a science teacher have grown exponentially in the last year.
One of the things I love about astronomy is the very fact that we are not laboratory-bound scientists. Our lab is the universe, a constantly changing petri dish in the sky, so to say, and if you aren’t looking, you miss it!
I believe having students work with other students from other schools has much value.
