Prize Recipient

Elizabeth Rose Fernandez

Background:

I have completed my freshman year at the New Mexico Institute of Mining and Technology where I am majoring in physics with a specialty in astrophysics. During the past year, I began work on a pulsar timing system that will be implemented at the Very Large Array (VLA). This summer I am working at the Starfire Optical Range, which is part of the Air Force Research Laboratory. Starfire is an observatory that employs adaptive optics, a system that uses a deformable mirror and lasers to remove the distortion from astronomical images caused by the Earth's atmosphere. Previously, I have worked on astronomical research projects during high school which earned me the 1999 National Young Astronomer Award. My first project measured the amount of cosmic radiation that the Earth receives whether shelter, altitude, time of day, or weather had any effect on the amont of incoming radiation. The following year I analyzed the spectyra of several galaxies to determine their shape, color index, distance, relative speed, and properties such as star formation or presence of a central supermassive black hole. For my final high school project, I observed and took CCD images of active galaxies in the Perseus Supercluster. I determined whether there where any differences between active an inactive galaxies and between the two types of active galaxies I found -Seyferts and LINERs. I found differences in the number of companion galaxies, peculiarities, presence of starlike nuclei, and significant differences in shapes of the galaxies.