Chelen Johnson
CM4Seyferts (Color-Magnitude for Seyferts): Using ultraviolet images from the Galaxy Evolution Explorer (GALEX) satellite and optical images and spectra from the ground based Sloan Digital Sky Survey (SDSS) to find a correlation between the color and luminosity of the hot gas around supermassive black holes at the centers of galaxies.
One evening, while working on some homework, I had the realization that THIS WAS REAL. There is no right answer, in fact, no one knows the answer. I can't just go and ask someone the answer. It was like a light bulb went off and I experienced a feeling of excitement and also felt a little bit scared. I thought to myself -- Is this how astronomers feel about their work? It was a great feeling and exciting that I too am part of this now.
[at the 2013 AAS,] I was always struck by the focus on ensuring the data is real and using modeling to create templates when classifying objects or processes.
I did not anticipate how much the astronomers would trust us right away. I felt more like a colleague than a student, which was relieving (and maybe a bit stressful, because I probably would have found it easier to ask questions coming from a student role).
