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.
I can't begin to tell you what a wonderful experience this week was for me and my students. The skills and knowledge we all picked up were great.
Sure, I wrote long papers for my masters', but those papers were to scholarship what engineering math is to actual mathematics - just get through it to do your job. Working with you in NITARP, I saw scholarship as a living community. [..] this experience encouraged me to write for the journal of my profession, but even moreso taught me to reach out to others[..]
For me, [this project] was a real partnership between scientists and educators. All questions and suggestion were taken seriously and with respect.
