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 NITARP experience has made me rethink my entire approach to science education. Many of my students expect me to do the work and pretty much hand it to them all wrapped up and neat. Science education must involve a great deal of discovery by the student and not a string of topics with definitions.
[NITARP] is a fabulous experience – I feel like after several years I am understanding more of the talks, able to engage in a real conversation with astronomers, ask questions one on one, interpret more on posters – just feel more astronomically literate.
I had an amazing, exhausting time at the [2012] AAS meeting. I found myself continually challenged by the intellectual level and knowledge being shared. I was surprised and very encouraged to see a high proportion of people which are generally considered underrepresented in the sciences. That was a terrific take-home message for my students. It was an excellent experience all around, and gives me confidence that my team and I will be able to do a good job with our project and be great representatives of the NITARP program.
