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.
To me what stood out [at my first AAS] was the wide variety of work – from characterization of the structure of the Milky Way (more of a challenge than I ever knew!) to the search for and characterization of exoplanets to the understanding of how quasar evolution relates to the origins of the Universe.
I did not anticipate how much the astronomers would trust us right away. I felt more like a colleague than a student, which was relieving (and maybe a bit stressful, because I probably would have found it easier to ask questions coming from a student role).
I cannot say enough positives about the NITARP experience for the participating students. They have had the opportunity to learn and grow and see science applied in authentic research projects while working with some of the coolest scientists around! It has allowed me to grow as a teacher and researcher and be able to share my insight and newfound knowledge with students and peers.
