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 rarely get out among other teachers in the same field as I am, with similar interest and motivations, and even less often do I have time to be in the company of professional scientists to see and hear what they are doing, how it is being done, what technologies are being used, etc. Without this type of program to get me to a meeting like the AAS I would never be able to put all of this together.
I had a request to present an inquiry professional development for educators while I was at NITARP and the AAS. Because of the amount of resources, new astronomy, lesson plans, and conversations I now feel I can try this with astronomy rather than my fields of practice.
Astronomers remain focused, polite, caring and thoughtful about the future generations who will take on the study. I think this message alone has huge meaning in my classrooms [...]
