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.
Science is hard! ;-) Also, it is worth the work!
Thank you for a life changing experience.
I have been a teacher for 38 years, and have been in probably 18-20 special programs over that time to improve myself as a science teacher. The NITARP program ranks as one of the three best programs I have been in over that period of time.
