Insights from Radio Wavelengths into Supernova Progenitors Laura Chomiuk Jansky Fellow, Michigan State University.
14-Jun-2004EVLA Software Design Review Transition Plan Bill Sahr 1 EVLA Hybrid Array & Transition Plan.
Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing.
A New “Radio Era” for Planet Forming Disks K. Teramura UH IfA David J. Wilner Harvard-Smithsonian Center for Astrophysics thanks to S. Andrews, C. Qi,
