Chelen Johnson
CM4Seyferts (Color-Magnitude for Seyferts): Using ultraviolet images from the Galaxy Evolution Explorer (GALEX) satellite and optical images and spectra from the ground based Sloan Digital Sky Survey (SDSS) to find a correlation between the color and luminosity of the hot gas around supermassive black holes at the centers of galaxies.
Every science teacher should get to go through a program like this.
Student involvement in authentic research is an idea whose time has come.
I already have more energy in the classroom and feel the need to pinch myself constantly.
