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.
This experience has forced me to look at something new and has inspired me to enrich and improve my classes.
Astronomers remain focused, polite, caring and thoughtful about the future generations who will take on the study. I think this message alone has huge meaning in my classrooms [...]
This has by far been the best professional development program I have ever been involved with.
