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.
Thank you for a life changing experience.
Having scientists explain their research and bringing it down to my level was very interesting and I learned so much!
This [whole NITARP] experience will help me understand how students feel when they are presented with new material and don’t understand. I think this will give me more patience and understanding in this area.
