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've enjoyed working with NITARP teachers and seeing just how talented they are and how passionate they are about what they teach and about their kids. They want to learn as much as they can here so that they can go and make their classrooms better.
I knew nothing about the online archives before this experience. Now I am quite familiar with them, and I have even used them a few times for reasons unrelated to NITARP. I am certain I’ll continue to use this resource going forward.
For the teacher, connecting with working scientists and networking with other colleagues has immeasurable value. I plan to utilize these relationships and potentially other projects spawned by them for years to come.
