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.
While a lot of astronomy is done by computer, nothing compares to having a human look over the data.
You really do become co-learners with the students.
What was especially important to me as an educator was the way that the students planned their own schedule of listening to research presentations [at the AAS] and reviewing poster presentations. The students were very active participants in the conference and they took away an amazing amount of information and excitement. One parent told me that her normally quiet son spent the entire weekend relating stories of the experience to his family and friends.
