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.
Your ongoing mentorship and availability is unbelievably valuable to me and my kids; NITARP is like a new chapter in my professional life.
[..]Students who are given the opportunity to do "real science" generally find a greater deal of success when it comes to understanding concepts (and at a deeper level).
Through this whole process I’ve learned that astronomy research is about connections. Who you meet, what they do, and how each has a part in a greater picture. Sharing information, connections and discussions.
