  We present the results from the on-going radio monitoring of recent type II
supernovae (SNe), including SNe 2004et, 2004dj, 2002hh, 2001em, and 2001gd.
Using the Very Large Array to monitor these supernovae, 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. Derived mass loss rates assume wind-established
circumstellar medium, shock velocity ~10,000 km/s, wind velocity ~10 km/s, and
CSM Temperature ~10,000 K.
