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.
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.
[The most interesting thing during the summer trip was] the change in the students and their growth in confidence. The a-ha moments when the big picture came into focus for them. The tour of
JPL was fantastic, too.
I wanted to share this with you about one of the students I had on our team that explored star formation in Lynds dark nebulae (LDNs) [in 2008]. [He has since become involved with a big Air Force program at Michigan Tech in 2012.] [He] has often thanked me for getting him involved in NITARP research, having used that experience, in part, to get access to programs such as MTU's Aerospace Enterprise.
