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 teachers who I have met through NITARP are just amazing. I am continually impressed by how hard they work and how enthusiastically they learn.
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.
One of the most interesting things I learned while working with my team was how unique and surprising each star can be.
