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.
Great to see real data taken from real telescopes take shape.
Our students, over the past few years since I participated in NITARP, have directly benefited from my being accepted into the program. You are a great asset and I appreciate all that you do!
