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 felt as if I was on a treasure hunt to identify new methods of confirming redshift values for our candidate cluster members.
While a lot of astronomy is done by computer, nothing compares to having a human look over the data.
Over all, the NITARP experience was nothing I had ever experienced before as a teacher. The research was very interesting and challenging at the same time.
