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 most interesting thing I did was to discuss the learning experience with the students who participated in last year’s project. Being in the final stage of their experience and reflecting on that process was the most fun for me. I truly enjoyed the sense of accomplishment they had gained while engaged in the experience. They were proud of themselves and seemed to be waiting for more.
I rarely get out among other teachers in the same field as I am, with similar interest and motivations, and even less often do I have time to be in the company of professional scientists to see and hear what they are doing, how it is being done, what technologies are being used, etc. Without this type of program to get me to a meeting like the AAS I would never be able to put all of this together.
I thought the talks and posters were great. Watching scientists talk to each other and question each other was interesting.
