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.
This week at Caltech was the greatest opportunity of my career. It was an experience that was humbling and at the same time gave me confidence. I cannot thank the NITARP program enough for the professional development, the professional relationships I've grown, and the inspiration. Thank you NITARP! Please keep this educational program going.
Overall, I think one of my favorite parts of the trip was watching all of the students from around the country bond into a very productive team. They would help each other through the work we were doing to make sure everyone understood and was at the same place.
[Because of a poster I saw at the AAS and] my participation in the NITARP program, I will be raising the standards for my students in the future.