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.
It was very special to be in the room when the announcement of planet Kepler 10b (an estimated 1.4 X the size of the Earth) was discovered. I turned to my student Inga and asked, "How does it feel to be one of the first people on planet Earth to know about this discovery?" She replied, "I never thought of it like that ... it's pretty cool."
I already had a pretty good idea of how astronomers do science, but NITARP helped me see more exactly how data is collected, processed, and analyzed. It helped me also see that I can do astronomy myself, and can make a contribution beyond my own classroom. Not only can I analyze astronomical data to find scientifically useful results, but I can publish my work as a poster and be part of this community. I did not feel like a stranger or usurper or even out of place – it felt like I belonged.
I have found that “real astronomy” involves a lot of data processing. In addition, I have found that collaboration is a very important aspect of the process.
