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.
I never met a scientist who did not want to discuss their work.
Honestly, I left [the 2013 AAS] a bit more in love with astronomy. I just plain had fun wandering and treated myself to time as a learner. It is not often we, educators, get to slide out of expert mode and into learner mode.
The more I talked with astronomers and support staff at the different booths [at my first AAS], the more I began to realize that being a teacher, and an amateur astronomer, is really very different from being a professional astronomer.
