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.
NITARP is without a doubt one of the two most valuable pieces of professional development work I have done in 25 years of teaching, and by far the most rewarding content-related work. I think that what you are doing is really unusual and valuable.
I’ve always thought that probably most astronomers were just normal people who had a passion for astronomy, and my experience confirmed that. I felt like many of the astronomers I talked to were able to have normal conversations as well as “wow” me with lots of data and analysis.
The NITARP experience inspires students to participate in research and inspires teachers to find a place in their work (either in a club, the classroom, or new programs) for authentic research. For me, personally, this year of working along with students to learn about black holes has shaped my pedagogical view that real research should be the basis for all science courses.
