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.
Found out that NITARP is bigger and better than I thought it would be.
Over all, the NITARP experience was nothing I had ever experienced before as a teacher. The research was very interesting and challenging at the same time.
My skills and knowledge as a science teacher have grown exponentially in the last year.