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.
In summary, this [AAS meeting] was amazing. For four straight days, if I'd thrown a rock I would have hit a scientist. Priceless.
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 assumed that [research] would require a great deal of data analysis, what I didn’t grasp until after this[, my first AAS] meeting was how focused and detailed the analysis would be. The steps in understanding that are gained through the analysis are much smaller than I anticipated they would be for the amount of work that is done.
