Chelen Johnson
Hertzsprung-Russel diagram for Active Galactic Nuclei (HR4AGN): Using space and ground based ultraviolet, optical, and infrared images to find a correlation between the color and luminosity of gas emission and dust emission around supermassive black holes at the centers of galaxies.
There was a connection for me, and I hope my students, between what at times can be very tedious number crunching and theoretical concepts to practical application of data towards discovery.
I just think experiencing a conference of this size and magnitude is terrific.
[..]this experience for the students was golden. Having the chance to share this opportunity for learning with my students is by far the best thing that came out of the project.
