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.
Watching the students present the research we had been working on the last year was absolutely the best part of the experience for me. They made me so proud
I have a much better sense of what research astronomy is about now, and I think I will have more confidence to try new things (related to astronomy) going forward.
I have learned that a student’s age or grade level can never be used to judge their ability to grasp the complex if they are only give the right time and instruction. They showed me that again on this trip.
