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 already had a pretty good idea of how astronomers do science, but NITARP helped me see more exactly how data is collected, processed, and analyzed. It helped me also see that I can do astronomy myself, and can make a contribution beyond my own classroom. Not only can I analyze astronomical data to find scientifically useful results, but I can publish my work as a poster and be part of this community. I did not feel like a stranger or usurper or even out of place – it felt like I belonged.
One thing I learned from this meeting is I love my project. It is going to be very interesting and way cool!! I can’t wait to tell my astronomy club about it.
I saw kids rise to a challenge and meet it – they learned a lot from the process, each other, and the experience – in ways they could not get in a regular classroom setting at home.
