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.
NITARP has been the best experience I have ever had for my personal and professional development as an astronomy educator.
I really enjoyed meeting members of the other NITARP teams and comparing their experience to mine. Everyone’s experience was different, but there seemed to be an overwhelming consensus that NITARP was the most significant, educational, and enjoyable professional development experience they have ever had. I could not agree more.
Every time we meet or talk or work on the project I feel just a little bit more knowledgeable, skilled and, perhaps most importantly, confident in what I know and can do...
