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 was surprised [during the summer visit] with the speed with which my students increased their proficiency with the tools we are using -- especially Python programming! My students acted very independently and hardly ever needed me to suggest something for them to do next; many times they were already anticipating the next tasks and trying to figure out how to do it!
I've been in the classroom for 35 years, and almost all science education, certainly through the high school level, is fact based and has nothing to do with how science is really done. The opportunity to actually participate in research from square one, where there's a question and no one knows how to answer it, but we're going to figure it out, was just so enticing.
For me, [this project] was a real partnership between scientists and educators. All questions and suggestion were taken seriously and with respect.
