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 "new" astronomy has become something we all knew was coming: handling huge chunks of data and learning how to mine this information from sets so large that it is simply mind boggling. The interesting thing is that many people are not aware of this, notably teachers in the trenches.
I think that my NITARP experience is one of the best things that I have ever done in my life, both as an educator and as an individual. I have found that I really like doing research and plan to continue that in the future both with my students and as an individual.
For me, [this project] was a real partnership between scientists and educators. All questions and suggestion were taken seriously and with respect.