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 reinforced to me the importance of learning science by doing science.
My ideas about astronomy has changed significantly, thanks to NITARP. Quite simply, I didn't understand the role of archival data in modern astronomical research. Previously, I considered it an intellectual exercise, work suitable for a reference librarian, but not real research. I now know it to comprise the future of astronomy, and the very picture of MOST of tomorrow's scientific research.
I was surprised and very encouraged to see a high proportion of people which are generally considered underrepresented in the sciences. That was a terrific take-home message for my students.
