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.
Before ever having experienced an AAS meeting, I thought I was well versed in the astronomer’s culture. [..] I also thought I knew what an astronomer did. [..] Well, this 221st meeting of the AAS has certainly been an eye opener. [..] My experience has been one of culture shock.
Your ongoing mentorship and availability is unbelievably valuable to me and my kids; NITARP is like a new chapter in my professional life.
Student involvement in authentic research is an idea whose time has come.
