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.
The time at Caltech was fantastic. I enjoyed working alongside my students in a way that felt very different from the typical classroom setting.
I did not anticipate the amount of people that were not "NITARP" but instead simply "fellow" astronomers and researchers that came by our team's poster to discuss our findings. That for me was [..] was a most pleasant surprise.
Real astronomy isn’t just looking through telescopes with the naked eye anymore. It is really being accurate and precise and a lot of computer mathematics.
