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.
The most interesting thing I did was to discuss the learning experience with the students who participated in last year’s project. Being in the final stage of their experience and reflecting on that process was the most fun for me. I truly enjoyed the sense of accomplishment they had gained while engaged in the experience. They were proud of themselves and seemed to be waiting for more.
I will definitely be using the skills and the knowledge that I acquired in the NITARP program in the future for my own and for my future students’ research.
I would advise the scientists to not be afraid of pushing the teachers and students outside their comfort zone. It’s ok if the teachers and students are struggling- we’ll catch up! Just go – make us work hard. It’s what we signed up for.
