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.
Thanks again for this amazing opportunity. I really hope it can continues even in light of the difficult financial times. It would be a terrible loss if it went away because it feels a very specific niche that is not met by any other program I have seen.
I really feel that NITARP is a gem of a program.
Overall, I think one of my favorite parts of the trip was watching all of the students from around the country bond into a very productive team. They would help each other through the work we were doing to make sure everyone understood and was at the same place.
