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.
[..]this experience for the students was golden. Having the chance to share this opportunity for learning with my students is by far the best thing that came out of the project.
The most interesting thing [during this whole NITARP experience] I did was work with catalogs I had not seen before and those I had that I had not a clue what to do with all that data. I now have a much clearer picture and my understanding has grown beyond what I think I could have ever done before.
Being there with my students was the most amazingly cool experience. I saw my two guys explode in their willingness to ask questions and express an opinion.
