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 really enjoyed meeting members of the other NITARP teams and comparing their experience to mine. Everyone’s experience was different, but there seemed to be an overwhelming consensus that NITARP was the most significant, educational, and enjoyable professional development experience they have ever had. I could not agree more.
This past year was a very intense NITARP experience for me, stretching my intellectual and technological skills beyond their limits while learning to be a mentor teacher and of course transferring as much of this experience to my students as possible.
Great to see real data taken from real telescopes take shape.
