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.
Having scientists explain their research and bringing it down to my level was very interesting and I learned so much!
This experience has made me conscious of how important it is to have students work with real data. I will definitely seek out more opportunities to include real data in my lessons and labs.
The best thing about the [Summer] trip was simply being on the campus at Caltech as an active participant in a science project. I still feel honored to be able to participate in this program. On top of that, to be able to extend the tendrils of my own learning to a few of my students only adds to the satisfaction I derive in being a teacher.
