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.
Because of NITARP my teaching has grown for the better. The entire project really made me appreciate and re-evaluate the scientific process. I was amazed by the support and well organized lines of communication, and found a new level of respect for Google Sheets.The number of connections I have made with other astronomy and physics teachers has really helped me find new and interesting ways to make physics more relevant to students.
The most interesting thing [of my NITARP experience] was having to actually do research – researching articles & known information; looking up images in databases; doing photometry; making judgments on sources.
I feel the NITARP experience will be a major influence for me here on out.
