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.
The experience I had at the 2012 AAS meeting as well as the entire NITARP experience will change the way I teach astronomy. Having spent 5 days meeting and discussing authentic scietific research with so many people from many different facilities was extremely rejuvinating as an educator.
This experience convinced me even further that I can push myself to learn even more each and every day. I started out feeling very overwhelmed and unprepared last year. I forced myself to work through my unease and wound up much more comfortable. I learned that astronomers are much more down-to-earth than I envisioned a lot of them to be and so many of them are very willing to go out of their way to explain things when we have questions.
The best thing about the [Summer] trip was simply being on the campus at Caltech as an active participant in a science project. I still feel honored to be able to participate in this program. On top of that, to be able to extend the tendrils of my own learning to a few of my students only adds to the satisfaction I derive in being a teacher.
