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 have been a teacher for 38 years, and have been in probably 18-20 special programs over that time to improve myself as a science teacher. The NITARP program ranks as one of the three best programs I have been in over that period of time.
Participating in NITARP has made me more confident about teaching Astronomy and communicating to students about how archive Astronomy research is done. They are surprised to learn that even THEY could do Astronomy research. My students and I had such a experience (they LOVED the JPL tour) and I'd love to participate again because I have some new students that I think would love this program!
I am gaining in confidence as to my ability to understand, contribute to the study, and the data we will be using.
