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.
So many of us science teachers do labs where the end is known (which is sometimes necessary to make sure they fit in a class period and that the students understand the concept we're trying to learn) but that's not really science.
Thanks again for this amazing opportunity. I really hope it can continues even in light of the difficult financial times. It would be a terrible loss if it went away because it feels a very specific niche that is not met by any other program I have seen.
The NITARP experience is truly phenomenal, and our scientist was wonderful to work with – never condescending and always very clear in his explanations.
