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 week at Caltech was the greatest opportunity of my career. It was an experience that was humbling and at the same time gave me confidence. I cannot thank the NITARP program enough for the professional development, the professional relationships I've grown, and the inspiration. Thank you NITARP! Please keep this educational program going.
I am gaining in confidence as to my ability to understand, contribute to the study, and the data we will be using.
I did not anticipate the amount of people that were not "NITARP" but instead simply "fellow" astronomers and researchers that came by our team's poster to discuss our findings. That for me was [..] was a most pleasant surprise.
