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’m thinking I’ll have my 6th graders each do a project on an observatory in our astronomy unit. There are so many!
One of my students at Niles West had become interested in GRBs as we thought they were the results of mergers of black holes [but we learned this was wrong at an AAS plenary talk]. My student thought it was interesting that scientists could change their minds about how things worked.
I enjoyed the whole week [at my first AAS]. The aspect that was best was connecting with my teammates. The personal contact at this early stage was important.
