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.
[..]Students who are given the opportunity to do "real science" generally find a greater deal of success when it comes to understanding concepts (and at a deeper level).
The most interesting thing I did was to discuss the learning experience with the students who participated in last year’s project. Being in the final stage of their experience and reflecting on that process was the most fun for me. I truly enjoyed the sense of accomplishment they had gained while engaged in the experience. They were proud of themselves and seemed to be waiting for more.
Working with teachers and astronomers across the country was great for my personal knowledge. Working across times zones was another fun, but interesting challenge. Learning how to work with completely new people, being in a new place, learning new material, all of these experiences help shape me better as a person.
