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.
Real astronomy is very exciting! I was not expecting to have to solve problems in excel the way we did. We were asked to answer simple questions or develop simple graphs at times but in order to get correct results (as far as we can tell) our team had to parse our skills and play with logic. I remember creating my first SED: I became so excited I could not sit down anymore. Another teacher was so thrilled they raised their hands and yelled in excitement. It was the first time we had results; it was a thrill.
I think the overriding theme of what new teachers need to know it that, yes, even though you are going to feel overwhelmed at times you need to sit back and enjoy the ride.
I assumed that [research] would require a great deal of data analysis, what I didn’t grasp until after this[, my first AAS] meeting was how focused and detailed the analysis would be. The steps in understanding that are gained through the analysis are much smaller than I anticipated they would be for the amount of work that is done.
