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.
Finally much of the [AAS 2009] invited talk by Eugene Churazov on Galaxy Clusters and Black Holes I found to be understandable because he used many equations from ideal gas laws that are familiar to high school teachers and their students. In talking with Dr. Churazov after his talk, he re-emphasized how far one could go on this topic with these familiar and seemingly simple equations.
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.
Participating in NITARP has made me more confident about teaching Astronomy and communicating to students about how archive Astronomy research is done. They are surprised to learn that even THEY could do Astronomy research. My students and I had such a experience (they LOVED the JPL tour) and I'd love to participate again because I have some new students that I think would love this program!
