Chelen Johnson
They Might Be Giants are using data from the Kepler mission to classify the brightness changes of giant stars in an effort to understand how the observed brightness variations of giant stars may relate to the different stages of giant star evolution.
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.
Being able to be physically present at Caltech and the AAS expanded the impact of this program significantly. It was in these settings, in particular, where one could see how the scientific enterprise typically works and how ideas are often shared.
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.
