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.
Thank you for opening such a wonderful door of opportunity for me. These two years have been the best professional learning experience of my career.
[Because of a poster I saw at the AAS and] my participation in the NITARP program, I will be raising the standards for my students in the future.
NITARP is the best!
