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.
[...]that provided a wonderful window into the student’s perspective of the NITARP experience. I loved how they talked about seeing math as a way of communicating and for checking data…not as THE right answer type computations. Many then said that concept was new and they really appreciated it.
I am excited to embark on this research and feel lucky to be part of the experience.
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
