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.
I am grateful for NITARP and appreciative for all those that put in the long hours so the program can be as successful as it is. I had heard about the program at a workshop in 2012 and decided to apply since I heard what a great program it is. My experiences have gone way beyond my expectations. Thanks [..] for giving teachers and students the opportunities you do!
This year [at the AAS] was so much different than last year [because of] having a poster to share with others!
Having scientists explain their research and bringing it down to my level was very interesting and I learned so much!
