Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
Finally much of the [AAS 2009] invited talk by Eugene Churazov on Galaxy Clusters and Black Holes I found to be understandable because he used many equations from ideal gas laws that are familiar to high school teachers and their students. In talking with Dr. Churazov after his talk, he re-emphasized how far one could go on this topic with these familiar and seemingly simple equations.
I cannot say enough positives about the NITARP experience for the participating students. They have had the opportunity to learn and grow and see science applied in authentic research projects while working with some of the coolest scientists around! It has allowed me to grow as a teacher and researcher and be able to share my insight and newfound knowledge with students and peers.
Real astronomy is very exciting! I was not expecting to have to solve problems in excel the way we did. We were asked to answer simple questions or develop simple graphs at times but in order to get correct results (as far as we can tell) our team had to parse our skills and play with logic. I remember creating my first SED: I became so excited I could not sit down anymore. Another teacher was so thrilled they raised their hands and yelled in excitement. It was the first time we had results; it was a thrill.
