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.
It is an eye opening and life changing experience for the participants.
I met a lot of people over the course of [my first AAS]. So many people were interested in chatting, especially with a high school physics teacher!
I’ve always thought that probably most astronomers were just normal people who had a passion for astronomy, and my experience confirmed that. I felt like many of the astronomers I talked to were able to have normal conversations as well as “wow” me with lots of data and analysis.