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.
It was very rewarding to be able to talk with astronomers who were willing to answer my (many) questions. Educators rarely have an opportunity to talk to professionals to hone their knowledge base once they finish school. I’m afraid I grabbed them every chance I got!
This has by far been the best professional development program I have ever been involved with.
I am gaining in confidence as to my ability to understand, contribute to the study, and the data we will be using.
