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.
This has by far been the best professional development program I have ever been involved with.
I thought the talks and posters were great. Watching scientists talk to each other and question each other was interesting.
[...]creativity has to be a underling personality trait for scientists
