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.
My takeaway lesson is that the students are much more tolerant of "issues" that make the research projects difficult to carry out and are generally content to be involved and learning something new.
I was nearly moved to tears watching the students share our research at the poster session.
Thanks so much for an amazing experience. NITARP has opened doors for me in many ways. It’s exposed me to real research, it’s got me thinking about ways to innovate and create real research experiences for my students, and it’s made me aware of the numerous opportunities out there for science teachers to become better at what they do.
