  The Cataclysmic Variable Section of the American Association of Variable Star
Observers (AAVSO) has initiated an observing campaign to study a subset of
dwarf novae (DNe), known as Z Cam type (UGZ). We call this program the Z
CamPaign. Since there is no strong agreement between the various published
catalogues as to which few dozen DNe are actually Z Cam type systems, our
primary goal is to accumulate enough data to construct detailed light curves,
covering the entire range of variability, to determine unequivocally the 30 Z
CamPaign subjects' membership in the UGZ class of DNe. We discuss the
organization, science goals, and some early results of the Z CamPaign in
detail.
