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.
I’ve always thought that probably most astronomers were just normal people who had a passion for astronomy, and my experience confirmed that. I felt like many of the astronomers I talked to were able to have normal conversations as well as “wow” me with lots of data and analysis.
I can't begin to tell you what a wonderful experience this week was for me and my students. The skills and knowledge we all picked up were great.
To be the first group to perform such calculations is an experience of a lifetime.
