We present results from the on-going radio monitoring of recent type II
supernovae (SNe), including SNe 2005cs, 2004et, 2004dj, 2003ed, 2002hh,
2001em, and 2001gd. Using the Very Large Array (VLA) to monitor these
supernovae at 1.3, 2, 3.6, 6 and 20 cm, we present their radio
light-curves.From these data we are able to discuss parameterizations and modeling and
make predictions of the nature of the progenitors based on previous
research. The National Radio Astronomy Observatory is a facility of the
National Science Foundation operated under cooperative agreement by
Associated Universities, Inc. Matthew Kelley and Brian Kaster are
undergraduates at Marquette University. KWW thanks the Office of Naval
Research for the 6.1 funding which supports his research.