My primary field of research is galaxy evolution, particularly through tracing the gas content and star formation activities over the cosmic time. Because most young stars form obscured by the gas and dust that gave their birth, I specialize in tracers in the infrared and radio wavelengths that can see through the obscuration. My technical training is in radio astronomy with a specialization in radio interferometry (VLA, ALMA), and I am currently the Project Scientist for the Large Millimeter Telescope, which is the collaboration between the University of Massachusetts and the country of Mexico.