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.
NITARP is a phenomenal opportunity. It’s the best thing I’ve ever done in terms of professional development. It’s fun working with teams from across the county.
When I look at how the intellectual process changed over the last year I imagine it going from a diffuse look at research and the entire conference experience to the extreme focus on our own project during the year and finally reaching outward again in Seattle to incorporate new information and understandings. Returning to AAS made the experience complete.
While a lot of astronomy is done by computer, nothing compares to having a human look over the data.