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.
By far, the most interesting part of my entire NITARP experience is the scientific method applied to the discovery process.
I can't wait to get started, and neither can my students!
Standing by the poster nearly all day, my three girls described our [research]. To say that I was proud would be a gross understatement.
