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.
The experience I had at the 2012 AAS meeting as well as the entire NITARP experience will change the way I teach astronomy. Having spent 5 days meeting and discussing authentic scietific research with so many people from many different facilities was extremely rejuvinating as an educator.
I found it most interesting to see the scientific process in action. Scientists were questioning scientists, sometimes fairly aggressively.
Just being exposed to the jargon is mind opening, and I can’t imagine walking into this convention and being asked to present without having this initial exposure. I think this [first AAS] trip is a crucial part of the program.
