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.
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.
I was looking for ways that my students and I could get involved with real science and real astronomy, and NITARP is doing exactly that.
In summary, this [AAS meeting] was amazing. For four straight days, if I'd thrown a rock I would have hit a scientist. Priceless.